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## (from tabmap V6.0 (2016-08-18)) 2024-05-21T16:08:20 #--------------------------------------------------------------------------- #-- II/250 Combined General Catalogue of Variable Stars (Samus+ 2004) #-------------------------------------------------------------------------- #---Table: II/250/./gcvs_rem.dat Remarks on GCVS stars (14441 records) # GCVS A10 --- Variable star designation # Text A81 --- Text of note. -------------------------------------------------------------------------------------------- GCVS |Text ----------|--------------------------------------------------------------------------------- R And |S5/4.5e. S And |SN (NGC 224). W And |S7.5/1-e. X And |S5/7-e. Z And |The light curve is characterized Z And |by outbursts up to 4m with intervals of 10 - 20 Z And |years. In the intervals cyclic variations are observed with Z And |the mean period of 632d and variations with cycles of Z And |several days and Delta(m) ~ 0.1m - 0.5m. The spectrum is Z And |symbiotic, with features of a late M giant, narrow Z And |low-excitation emission lines (Bleq) and forbidden lines Z And |characteristic of highly excited nebulae. RR And |S6/3.5e. RT And |Min II 8.88; DI = DII = 0.17P; dI = dII = 0.00. P var. RT And |Nonlinear term: -6.33*10**(-11)*E**2. During RT And |JD2433477 - 43878 linear elements are satisfactory: RT And |Min = 2441141.8888 + 0.62892984d*E. Period changes RT And |according to a sine law are possible [08002]. RU And |P var. Max = 2419857 + 243.0d*E (JD2412800 - RU And |20000); Max = 2434551 + 233.24d*E (JD2420000 - RU And |34550). Since JD2435000 - see Table. Delta(m) ~ 4m - 5m RU And |(before JD2429600), ~1m (JD2429600 ~ 33600), up to 3m RU And |(JD ~2436000), ~1.5m (JD ~2436700). In 1970 - 1972 RU And |showed quite irregular variations. RX And |SB (P = 0.21173d). Cyclic variations with P ~ 38s - 54s RX And |were observed after a normal maximum; after a short RX And |maximum no periodicity was found [08004]. SS And |Two long period variations are also observed: SS And |P = 650d, P = 3800d. ST And |P var. Max = 2418370 + 337.3d*E (JD2418000 - 28000). ST And |Since JD2428000 - see Table. SU And |VB A (B 12.77m V, F0V:, 15"). SV And |The magnitude in Max varies periodically, P = 930d, SV And |P = 5400d? [02146]. SW And |[Fe/H] = +0.16. P var. Nonlinear term: SW And |-1.229d*10**(-10)*E**2 [01959]. Since 1959 SW And |Max = 2436466.828 + 0.442270121d*E [06929]. SW And |The shape of the light curve varies with SW And |Pi ~36.83d = 83.28 P. The deviations (O - C) satisfy SW And |the elements of Blazhko effect SW And |Max(O - C) = 2436816.23 + 36.921d*N. Secular trend SW And |and cyclic (P ~2a) variations of (O - C) are possible SW And |[08005]. SY And |d = 0.027P. TT And |Min II 11.6? TU And |P var (Pi ~37a?). TV And |P var? Delta(m) strongly varies. TW And |d = 0.020P. Min II 8.94. P var. Min = 2428845.422 + TW And |4.122739d*E (JD2420050 - 32000). Since JD2432000 - see TW And |Table. TZ And |P1 = 118d: [00882]. TZ And |Mean magnitude varies with P2 = 974d [00098]. P = 135d TZ And |(JD2437545 - 38377) [03367]. UU And |P var. Min = 2428832.536 + 1.486311d*E (JD2421455 - 23740) UU And |[02262]; Min = 2428832.465 + 1.48629d*E (JD2428830 - 35012) UU And |[00745]. Since JD2441100 - see Table. UW And |P var. Before JD2430000 Max = 2418585 + 236.7d*E. Since UW And |JD2436000 - see Table. WW And |d = 0.012P. WX And |P var. Max = 2422613.614 + 3.0012544d*E (JD2422610 - 34712) WX And |[01240]. The Table gives current elements. d = 0.03P WX And |in 1972 and probably varies. WZ And |Min II 11.9. P var [02262]. Min = 2435075.342 + 0.695662d*E WZ And |(before JD2440500); probably WZ And |Min = 2440872.290 + 0.6956576d*E since JD2440500. WZ And |The elements in the Table represent all the observations WZ And |satisfactorily. XX And |P var. Max = 2418001.938 + 0.7227486d*E (1908 - 1932); XX And |Max = 2427106.403 + 0.7227591d*E (1932 - 1946) [02264]. XX And |Since 1946 - see Table. Delta(S) = 9. Blazhko effect: XX And |Max = 2437578 + 36d*N [03111]. XY And |Blazhko effect is possible. XZ And |Min II 10.16; DII = 0.26P. P var [02431,06932,08008,08593] XZ And |Min = 2432883.6046 + 1.3572708d*E (JD2431700 - 36150) XZ And |[01977]; Min = 2441954.340 + 1.357293d*E XZ And |(since JD2436200). The elements in the Table represent all XZ And |the observations satisfactorily. AA And |Min II 10.5. AB And |Min II 10.20. P var. Period increased suddenly in 1953 AB And |( ~JD2434500); no period changes later [02509,05222]. AB And |Elements since 1953 - see Table. AC And |Unusual multiperiodical variable. Second oscillation: AC And |Max = 2432467.373 + 0.71124243d*E; P3 = 0.421069d [08187], AC And |see also [08294,08295]. Delta(S) = -1:. AD And |Min II 11.6. Depth of minima in yellow light: 0.62m (Min I), AD And |0.58m (Min II) [03141]. Min II - Min I = 0.494P. P var. AD And |Min = 2428718.402 + 0.9861940d*E (JD2417460 - 29640) AD And |[01983]. Since JD2428700 - see Table. AE And |In the M31 galaxy. Strong UV continuum. AE And |Emissions: H, He I, Fe II, [Fe II]. AF And |In the M31 galaxy. Strong UV continuum. AF And |Emissions: H, He I, Fe II, [Fe II]. AG And |According to [08296], DSCT:, Min = 2442636.5868 + 0.0347d*E, AG And |A = 0.5m. AM And |VB A (B 0.25' S). AN And |Min II 6.09. The existence of the third body in AN And |the system is possible. Sp(Met) = F2 - F5. AP And |Min II 11.9. The period may be 2 times shorter. AT And |B - V: +0.42, +0.56. Delta(S) = 3. See [08299] for data AT And |on period variations and a detailed study. BD And |Min II 11.4. BE And |Average cycle: 137d [01993,02267]; 156.8d after JD2431700. BL And |Depth of Min II 0.24m: P var? Min I = 2429491.255 + BL And |0.7223779d*E (JD2415800 - 33900) [01995]. Since JD2433900 - BL And |see Table. BX And |ADS 1671 A (B 9.7m, 20", 59deg). Min II 9.15. Possible BX And |period change from 0.61011222d to 0.61011534d (~1952). BX And |On the period changes see also [08657]. BY And |According to [08658], SRB:. CC And |Possibly in a binary with Porb = 10.469d. Delta(m) and the CC And |light curve shape vary with a period 5.23714d or 10.469d CC And |[08016]. According to [03120], 4 periods are present: CC And |P2 = 0.0632083d. First overtone was not found. Other CC And |periods are resonances. CG And |P var: 3.7430d (1950), 3.7394d (1963) [05224]. CG And |Cyclic period changes are possible. CG And |According to [06941], short period oscillations (P = 2h 04m) CG And |are present. A number of observers do not find short-term CG And |variability. CM And |According to [00821], Max = 2428380 + 140d*E and Max = CM And |2430616 + 124d*E, and the star resembles UU Her. CN And |Min II 9.96. CO And |d = 0.06P: CP And |d = 0.01P? Depth of Min II 0.05m? CU And |d > 0.034P ([06943], according to visual observations.) DI And |DCEP? [03165]. DK And |EW? DL And |In the field of the open cluster NGC 7686. DR And |P var. Before ~JD2437000 Max = 2436078.384 + 0.5630609d*E DR And |[02275]; then P changed abruptly. Delta(m) changes by ~0.3m, DR And |Max A1 = 2436078.8 + 69.486d*N1, Max A2 = 2437646.65 + DR And |69.719d*N2. Other possible cycles are 2000d (interaction DR And |of cycles N1 and N2) and ~30 years [08019]. DS And |In the field of the open cluster NGC 752. Min II 10.7. DZ And |According to [04008], type RCB, spectrum R. According to DZ And |[06945], since 1961 is in Max light all the time. According DZ And |to [06946], the spectrum is not characteristic of RCB stars. DZ And |According to [08660], the star was bright near the moments DZ And |of Min light given in [04008]. EG And |P = 40d or 80d [08020]. EG And |Absorption spectrum with overlaying emissions of high EG And |excitation [04434,08598]. Strong variable magnetic field EG And |[04435]. Long period variations of light are observed. EG And |Radial velocities profiles and equivalent widths of lines EG And |vary with P = 470d [08596] (SB? [08597]). Possibly is EG And |analogous to HM Sge [08598]. EH And |IR excess. The presence of a dust envelope is possible. EO And |Very red. EP And |Min II 12.5. ET And |Delta(B) = 0.035m, Delta(U) = 0.07m. ET And |The Table gives the epoch of Max light. Observations may ET And |be represented by the periods 0.723d and 1.61553d ET And |[08022,07946]. According to [08023], in June - December 1977 ET And |Min = 2443337.4725 + 0.49925d*E, other periods are ET And |not satisfied by observations. According to [08599], ET And |Max(U) = 2439751.28 + 0.617135d*E (1967 - 1971). ET And |SB, Max(Vr) = JD2443718.0 + 48.304d*E [08301]. ET And |Photometric periods could not be found in radial ET And |velocities. EX And |Possible Min II 13.0:, Min II - Min I = 0.55P. EY And |I - K = 5.38; EY And |the presence of a dust envelope is possible [06947]. FF And |10.35m - 10.42m V outside flares; M - m = 0.50P. FF And |Porb = 2.170304d [08024]. According to photometric FF And |observations, P = 2.14d (1971), P = 2.15d (1972), FF And |P = 2.19d (1973) [06948]. FG And |According to [04156], EA; Min = 2436074.528 + 0.99772d*E. FL And |d = 0.02P. FZ And |mu = 1", p = 64deg. GK And |Min II 11.5. GN And |ADS 409 A (B 13.3m, 2", 6deg; C 11.6m, 141", 130deg). GN And |Different authors give spectral types F0 III, F2V, Am GN And |(probably based on different criteria). GP And |Delta(m) changes with P2 = 0.64d. GP And |A wave with P3 = 0.012161d is present. The mean GP And |magnitude and the shape of the light curve vary GP And |[08302]. GQ And |ADS 246 B (A = GX And; B 37", 61deg). B - V = +1.80. GQ And |X-ray source. GR And |Min (magnet.field) = 2442288 + 525d*E. GR And |Magnetic field varies (-250 to -1030 Gauss). Period of GR And |changes of C1 is near 1.5 years [07893]. According to [06257], GR And |period of changes in u is near 1 year or longer. GS And |B - V = +1.7 in normal light. GX And |ADS 246 A (B = GQ And, 37", 61deg). Delta(U) = 0.55m. SB? GX And |(conflicting data). GY And |SB1 (P = 273.2d [07324], P = 272.99d [08303]). GY And |For spectral changes, variations of light and magnetic GY And |field it is possible that P = 23a [07004] or 20.60a [08303]. GY And |[08022] gives P ~36.5d and Delta(V) ~0.049m. Periods 4.92a GY And |and 1.8d may exist [08303]. GZ And |B - V: +0.77, +0.82. ADS 1693 A (B 11.13m, 8", 31deg). GZ And |Min II 11.58. P var? GZ And |The period is based only on Minima I [06830] and GZ And |was improved with account of recent data. HH And |Subdwarf? [06581]. mu = 1.82", p = 176deg. HI And |B - V = 1.8m outside flares. HN And |Max(U) = 2438327.8 + 69.433d*E [08022]. SB HN And |(P = 106.27d [07435]). HQ And |According to [08659], a probable cataclysmic binary; HQ And |similarity to AM Her and AN UMa is noted. HR And |d = 0.05P. HT And |B - V = +0.60. In the region of M 31. HU And |Min II 17.2. In the region of M 31. HV And |According to [08659], a probable cataclysmic binary; HV And |similarity to AM Her and AN UMa is noted. HY And |In the region of M 31. HZ And |In the region of M 31. P > 100d. Red. IL And |d = 0.02P. IM And |In the region of M 31.8. IO And |According to [08659], a probable cataclysmic binary; IO And |similarity to AM Her and AN UMa is noted. IP And |d = 0.02P:. KK And |The light curve has double-wave shape KK And |[07740]. Long period variations were found [07955]. KU And |I - K = 4.63. KU And |SR type is possible. Surrounded with a dust envelope [08029]. KX And |SB2 (P = 38.908d). KZ And |ADS 16557 B (A 7.0m; B 15", 254). LM And |Min II 12.7. LN And |Delta(B) = 0.025. LO And |Min II 11.82. V0369 And |VB (0".1, 128 deg, 1986.9). V0374 And |Not identical with BD+44 422. alf And |SB (P = 96.6960d). VB A (B 11.2m, 80"). alf And |Epoch of Max U light is given. alf And |Hbeta index varies in the range of ~0.02m with P alf And |~3h [08030]. Rapid rotation. zet And |Depth of Min II 0.1m. SB. zet And |Unstable light curve. Most notable zet And |variations on the rising branch of Max II [08030]. zet And |Many peculiarities in the spectrum. lam And |SB1 (P = 20.52d). omi And |v sin i = 300 km/s; VB(0.3"; possibly omi And |also 0.05" - according to speckle-interferometric data). omi And |Shell spectrum appeared and disappeared several omi And |times since 1890. Different authors attributed omi And |the star to EB type. According to [05955], The changes omi And |of light may be explained also by intrinsic omi And |variations of a single shell star. They are represented omi And |by elements: Min I = 2439470.628 + 1.0185d*E. omi And |According to [02572], Min I = 2436174.430 + omi And |1.5998398d*E. The periodogram analysis shows omi And |a stable peak at P ~0.84d [08032]. A possible shell omi And |event was observed late in 1975. S Ant |Min II 6.87. P var? T Ant |CWB? P var. [A/H] = -0.0. P = 5.9098d (JD2428187 - T Ant |34688), P = 5.8976d (JD2434688 - 37660) [05387]. T Ant |The Table gives mean elements which satisfy all T Ant |observations well enough. V Ant |OH, H2O maser. Z Ant |Mean brightness varies with P = 1143d. SW Ant |Min II 14.6. UZ Ant |P var? WY Ant |P var. P = 0.57430871d (JD2414000 - 22070); P = WY Ant |0.57431618d (JD2422070 - 25600); P = 0.57431216d WY Ant |(JD2425600 - 29000) [01113]. (k - b)2 = 0.00. WZ Ant |Min II 11.8. XX Ant |Min II 9.1. XY Ant |Depth of Min II 0.3m - 0.5m pg. XZ Ant |Min II 10.2. Z Aps |Possibly also an eclipsing binary. RT Aps |Strong variations of period and the shape of RT Aps |the light curve [06152]. TY Aps |Delta(S) = 3. YY Aps |The period is probably long. AF Aps |Min II 13.9. AN Aps |Min II 12.8. AP Aps |Min II 15.5. AS Aps |Min II 13.8. AV Aps |Depth of Min II 0.05m. CE Aps |P = 209d or 261d. CY Aps |Min II 13.0. EF Aps |Min II 12.6. FY Aps |Deep Min II. GK Aps |Min II 13.9. RRC type is possible. GO Aps |Min II 14.8. RR type is possible. GQ Aps |Min II 14.8. GU Aps |Min II 14.5. GX Aps |RV type is not excluded. The epoch of Min is given. GY Aps |Min II 14.2. HL Aps |Min II 12.6. HO Aps |Min II 13.7. HT Aps |Min II 14.3. HV Aps |Epoch of Min is given. HX Aps |Min II 14.4. II Aps |Min II 11.6. IL Aps |Epoch of Min is given. IO Aps |Min II 12.4. IR Aps |Min II 13.8. IU Aps |Min II 14.6. IY Aps |Min II 12.9. KN Aps |d ~0.03P. KR Aps |Possibly a slow eclipsing variable. KT Aps |Min II 15.2. KV Aps |Min II 13.6. KZ Aps |Smooth light KZ Aps |changes with superimposed variations of eclipsing KZ Aps |nature, with minima on JD2436729 and 2436808. LM Aps |RV type is possible. LN Aps |Min II 13.3. LO Aps |Min II 11.5. MY Aps |L19-2. P0 = 192.75s, P1 = 113.77s. del 1 Aps |In a wide pair (delta2 Aps, 100", common mu). kap 1 Aps |SB? VB A (B 11.27m V, 27"). R Aqr |Symbiotic spectrum. Emissions of H, SII, OIII, FeII, NeIII, R Aqr |OII. Variable radio source. SiO maser. The secondary may R Aqr |be an accreting white dwarf. The star is embedded in an R Aqr |expanding gaseous nebula several hundred years R Aqr |old. A cycle ~24a and longer-term variations are R Aqr |possible in the changes of radial velocities and period. U Aqr |Strong bands of 12C2, CN, U Aqr |lines of SrII, YII in the spectrum; hydrogen deficiency. U Aqr |A probable halo star (Vr ~100 km/s.). Z Aqr |1969 - 70: P = 100d +- [05973]. RY Aqr |P var. Min = 2433872.352 + 1.966598d*E (before RY Aqr |JD2428000); Min = 2440824.410 + 1.966620d*E RY Aqr |(JD2428000 - 41000); Min = 2440824.410 + RY Aqr |1.966611d*E (JD2441000 - 43800). Since RY Aqr |JD2443800 P = 1.966554d? RY Aqr |The Table gives elements representing RY Aqr |observations after JD2428000 with the accuracy +-0.1d. ST Aqr |Min II 9.37. P var. Min = 2423640.271 + 0.78101367d*E ST Aqr |(JD2423500 - 26000) [02037]. Since JD2439700 - see Table. SU Aqr |ADS 16318 A (B 10.7m, 5", 144deg). Min II 10.5. P var? SV Aqr |Cycle 200 - 300d is possible. SW Aqr |P var. (k - b)2 = 0.01. SX Aqr |P var? Delta(S) = 9. SZ Aqr |Epoch of Min is given. TT Aqr |VB A (B 15m, 3", 135deg). TZ Aqr |Delta(S) = 5. VY Aqr |Second outburst: Max ~JD2437897 VY Aqr |(1962), ~9m pg [03129]. WX Aqr |Blazhko effect is possible. XZ Aqr |P var. Before JD2437913 P = 2.059187d. YZ Aqr |B - V = 0.49 (in Min). (k - b)2 = 0.06. YZ Aqr |Small fluctuations of period are possible. AE Aqr |Unusual flare X-ray system with pulsar. Becomes bluer AE Aqr |in Max. In Min B - V = +0.92. Shows rapid irregular AE Aqr |variations, which differ it from UV stars and UG AE Aqr |system, though the spectra are somewhat similar. AE Aqr |Simultaneous photoelectric and spectroscopic observations AE Aqr |[03131] show the existence of two types of flares: AE Aqr |1) intensification of emission lines accompanied by AE Aqr |brightening in U and B; 2) intensification of continuum AE Aqr |leading to brightening in U, B and V ("white flare"). AE Aqr |Detailed spectroscopic investigation [01971]. AE Aqr |Porb = 0.41165794d + 1.12*10**(-10)*E, The epoch AE Aqr |T0 = JD2439030.621 [08672]. In the X-ray band AE Aqr |(0.1 - 4.0 keV) pulsations with P = 33.0767s are observed AE Aqr |[08673]. In the optical range pulsations with AE Aqr |P0 = 33.076737s as well as with P1 = 16.5s were noted AE Aqr |[08674,08675]. AT Aqr |Min II 14.7. AX Aqr |P var. Before ~JD2427367 Max = 2425417.60 + 0.388135d*E AX Aqr |[03113]. AY Aqr |Min II 14.3. BH Aqr |P var. Before ~JD2431150 Max = 2426948.411 + 0.5258022d*E BH Aqr |[03113]. BI Aqr |Min II 13.1. BK Aqr |Close companion. BL Aqr |Waves from 80 to 125d. Mean magnitude changes BL Aqr |with cycles from 480 to 700d in the range of 0.3m - 0.6m. BM Aqr |The mean magnitude may vary with P = 500 - 600d. BN Aqr |Delta(S) = 4:. P var. Before JD2428964 Max = BN Aqr |2426577.901 + 0.46963401d*E [03113]. BN Aqr |According to [05391] Max = 2429395.742 + BN Aqr |0.4696410d*E + 3.3*10**(-10)*E**2 (1898 - 1958). BO Aqr |P var? (k - b)2 = 0.01. BQ Aqr |d = 0.07P. BR Aqr |P var? (k - b)2 = 0.16. BS Aqr |Delta(S) = 0. P var? BT Aqr |B - V: +0.14, +0.52. P var. Blazhko effect. BV Aqr |P var. Blazhko effect with Pi = 11.56d and variations of BV Aqr |light in Max up to 0.75A. BW Aqr |d = 0.01P. Min II 10.8. Min II - Min I = 0.484P. BW Aqr |Jensch [00189] considers the secondary Min to be the BW Aqr |main one. BX Aqr |d = 0.027P. CD Aqr |d = 0.012P. Min II 10.2. CE Aqr |According to [02548], no CE Aqr |variations were found in visual observations during CE Aqr |several months in 1954 - 1958. According to [03138], CE Aqr |the star may be analogous to AI Vel; P = 0.16d? CH Aqr |P var? CI Aqr |Period may be twice as long. CM Aqr |Min II 13.6. CP Aqr |Delta(S) = 3. CR Aqr |Min II 14.2. CV Aqr |Minor planet (52) Europa. CW Aqr |Min II 10.8. CX Aqr |Min II 10.8. Broad hydrogen lines. CY Aqr |Delta(S) = 2. P var; abrupt change ~1952. Before JD2434000 CY Aqr |Max = 2434308.4314 + 0.061038509d*E. The shape of CY Aqr |the light curve probably varies. For M - m different CY Aqr |authors give values from 0.23p to 0.40p. Beat phenomenon CY Aqr |with P2 = 0.2182d is possible [08060]. CZ Aqr |Min II 11.1. Cyclic variations of period? DD Aqr |Min II 11.2. DN Aqr |(k - b)2 = 0.01. DO Aqr |P var. DS Aqr |P var. DV Aqr |Min II 6.1. SB. In [08061] variations were noted DV Aqr |with Delta(m) ~0.1m and P < 3h, presumably of DSCT DV Aqr |type nature. Some sources give A3 for the spectral DV Aqr |type. Shell spectrum was observed in May, 1975. DV Aqr |Spectral lines were filled with emission and therefore DV Aqr |weak, strong absorption in H and K CaII lines was present. DV Aqr |Shell effects were not present in the spectra taken in DV Aqr |1971 - 1973 [08062]. DX Aqr |VB B (A 7.0m, K0III; B 3.7", 244deg). SB1. d ~0.015P. DX Aqr |Depth of Min II ~0.3m. DX Aqr |The range of combined brightness is given. DY Aqr |d = 0.04P. EE Aqr |Min II 8.48. EK Aqr |Min II 11.23. EL Aqr |P = 0.6345d is possible. EM Aqr |According to [06204] P = 0.068d. EM Aqr |Period and amplitude vary on very short time EM Aqr |scale. Light and colour vary approximately in phase. EM Aqr |The beat period, if exists, is shorter than 1d. ET Aqr |Period is given according to [08336]. EW Aqr |Delta(m) varies. FF Aqr |d = 0.059P. SB1. The unique eclipsing system of a red FF Aqr |star and probably a blue hot subdwarf. The amplitude of FF Aqr |the eclipse is 0.15V, 0.4B, 1.2U. The magnitude in Max FF Aqr |varies by 0.35V, 0.33B, 0.22U. Variable shape of light FF Aqr |curve. Strong emissions H and K CaII, Halpha in the FF Aqr |spectrum. FI Aqr |Possibly P = 4.659d or 4.719d. Epoch of min is given. FK Aqr |BDS 11854 A (B = FL Aqr, 11.45m, 24", 352deg, 1966). FK Aqr |mu alpha = +0.455", mu delta = -0.067". SB2 (P = 4.08322d FK Aqr |[00313]). Flares Delta(U) = 0.7 [00344]. FL Aqr |BDS 11854 B (A = FK Aqr; B 24", 352deg, 1966). KV Aqr |One deep fading overlapping a brightening trend. omi Aqr |Shell or disk spectrum is observed. pi Aqr |The brightness increased by ~0.2m V pi Aqr |in 1957 - 1975, the star became redder. Balmer pi Aqr |continuum in emission. Rapid changes in emission pi Aqr |lines and in polarization. Existence of a disk pi Aqr |or a shell is possible. R Aql |P var. Max = 2440038 + 297d*E (JD2427850 - 40000). R Aql |Since JD2440000 - see Table. R Aql |For the whole observed period R Aql |Max = 2399190 + 346.932d*n - 0.239303d*n**2; R Aql |Pn = 348.980d - 0.554202d*n + 0.000552309d*n**2 [03143]. R Aql |H2O, OH and SiO maser. Radiobursts. U Aql |B - V: +0.84, +1.24. P var. ADS 12503 A (B 14.00m, U Aql |35", 349deg, 1900; one more companion 11.7m V, 2", 230deg, U Aql |1934). W Aql |S 6/6e. Composite spectrum near Min light; a companion W Aql |(F5 - F8) may exist [03502]. Y Aql |Depth of Min II 0.03m. SB1. RR Aql |Maser H2O, OH, SiO. RT Aql |Maser H20, OH, SiO. SY Aql |Maser H2O, OH. SZ Aql |B - V: +1.04, +1.82. P var [02392]. Before JD2420260 SZ Aql |P = 17.1359d. Current elements - see Table. TT Aql |B - V: +0.96, +1.62. P var. [02392]. Before JD2418035 TT Aql |P = 13.7518d. Current elements - see Table. TV Aql |P var (changed at ~JD2430000). TV Aql |Before JD2430000 Max = 2429730 + 237.9d*E. TW Aql |Cycles 65d or 95d are observed during different time TW Aql |intervals [08714]. UU Aql |Mean cycle: 71.3d [04063]; 56d [03144]. UY Aql |Cyclic changes of light (P ~400d) with superimposed very UY Aql |rapid variations are noted in [00504]. VX Aql |SC5-/8e. According to [04231], the variable is irregular. VX Aql |Lithium star. VZ Aql |B - V: +0.61, +1.01. XZ Aql |P var. Min = 2424449.277 + 2.139147d*E XZ Aql |(JD2424380 - 2430300). Since JD2433000 - see Table. YZ Aql |d = 0.03P. P var. AA Aql |Delta(S) = 1.0. AC Aql |P var. AD Aql |CN bands are observed in the spectrum. According to [06928], AD Aql |the range is 8.83 - 13.42 V. AE Aql |VB A (B 16.6m, 12", 330deg; C 16.9m, 11", 0deg). AE Aql |The combined light of A, B, C varies in the range AE Aql |13.9 - 15.8. AF Aql |The period may be two times shorter. AL Aql |d = 0.04P. AU Aql |According to [03146], P = 190d or 380d. BL Aql |P var. Max = 2418538 + 159.65d*E (JD2418529 - BL Aql |29075). During JD2436420 - 38940 - see Table. BY Aql |P var? CD Aql |Close companion? CL Aql |Sometimes maxima predicted according to the CL Aql |elements do not occur. CM Aql |Symbiotic spectrum similar to that of Z And [03149]. CR Aql |Considerable Blazhko effect is possible. CS Aql |Close companion? CT Aql |According to [06004], only slow irregular variations with CT Aql |Delta(m) ~0.6 were observed in 1963 - 1968. CU Aql |P var? (Possible change ~JD2423000). Earlier Max = 2418591 CU Aql |+ 203.7d*E. CV Aql |P var? CW Aql |Close companion? DD Aql |Close companion? DT Aql |P var (Change ~JD2425000). Earlier Max = 2423964 + 290.5d*E. DY Aql |P var [06107]. EV Aql |P var. Before JD2423900 P = 38.67d. [A/H] = -0.3. EX Aql |P = 117d is also observed. EZ Aql |P var [06107]. FF Aql |ADS 11884 A (B 10.37m, 7", 141deg). SB1 (P = 1435d). FG Aql |At the edge of the dark nebula Barnard 130. May be a FG Aql |physical pair with FH Aql (rho ~20"). According to FG Aql |[00504], the mean cycle of light variations is 3.5d. FG Aql |The level of mean light varies. FH Aql |At the edge of the dark nebula Barnard 130. May be a FH Aql |physical pair with FG Aql (rho ~ 20"). According to FH Aql |[00504], the mean cycle of light variations is 3.44d. FK Aql |Depth of Min II 0.03m. P var. FM Aql |B - V: +1.12, +1.50. FN Aql |B - V: +1.10, +1.39. P var. FZ Aql |VB A (B 11.5m, 14", 162deg). GM Aql |UV type is possible [00504]. GU Aql |d = 0.02P. GV Aql |Nova-like star according to [02089]. GY Aql |Maser OH, SiO. HK Aql |Type ISB is not excluded. HL Aql |P var? The 15m star shown in the charts [02274,06996] with HL Aql |co-ordinates coincident with those given at the discovery HL Aql |is constant according to [02274]. IM Aql |P var. Before JD2432772 Max = 2428064.707 + 0.4569602d*E. IO Aql |VB A (B = IP Aql, 30", 101deg). IP Aql |VB B (A = IO Aql). IS Aql |Close companion. KL Aql |B - V: +0.78, +1.19, [A/H] = 0.6. KO Aql |d = 0.018P. Min II 8.40. P var. Min = 2427550.565 + KO Aql |2.863859d*E (JD2426250 - 33000) [02462]; Min = KO Aql |2433888.366 + 2.863954d*E (JD2433000 - 39000). KO Aql |current elements - see Table. KP Aql |Min II 10.43; Min II - Min I = 0.50P; DII = DI. KV Aql |During JD2429130 - 31370 - see Table. KV Aql |During JD2428308 - 28433 the star was faint. Max 2436015 KV Aql |also is not satisfied by the elements. LU Aql |In [03158] P = 102d is given, and the existence of the LU Aql |variation of mean magnitude with P ~1080d and LU Aql |Delta(m) = 0.4m was suspected. MV Aql |Close component, the range is given for combined light. NN Aql |Cyclic P variations? NV Aql |Variations of mean light with P ~ 900d - 1000d and NV Aql |Delta(m) ~0.6m. OO Aql |Min II 9.8. P var. Min I = 2426892.0582 + OO Aql |0.5067954d*E (1932 - 1934), Min I = 2433925.3762 + OO Aql |0.5067943d*E [08072]. Since JD2438000 - see Table. OO Aql |The shape of the light curve varies. OX Aql |Var 2 in the chart for OW Aql. PP Aql |[A/H] = -0.0. CWA type PP Aql |is not excluded. According to [03161] PP Aql |P var. Max = 2415229.15 + 24.0147d*E (JD2415228 - PP Aql |21064), Max = 2426576.14 + 24.074d*E (JD2426576 - PP Aql |29489). After JD2432040 Max = 2433141.78 + 23.994d*E. PP Aql |Current elements Max = 2436836.04 + 23.973d*E. PZ Aql |P var? According to [05387], before JD2428075 P = 8.7555d; PZ Aql |P = 8.7504d (JD2428075 - 34725); since JD2434725 PZ Aql |P = 8.7573d. See also [02274]. Elements in the Table are PZ Aql |satisfactory after JD2433150. The shape of the light curve PZ Aql |apparently varies. QS Aql |Min II 5.97. VB (A 6.5m; B 6.7m, 0.18", 137deg). P var. QV Aql |The epoch of main Max is given. QY Aql |d = 0.016P. P var? V0336 Aql |B - V: +1.17, +1.55. V0337 Aql |Min II 9.09. P var. V0337 Aql |The shape of the light curve varies. V0340 Aql |d = 0.05P. P var. V0341 Aql |P var. Delta(S) = 4. V0342 Aql |ADS 12259 B (A 7.5m; B 20", 14deg); d = 0.032P. P V0342 Aql |increases (see also [02265,04493]). Before JD2435600 Min = V0342 Aql |2428023.550 + 3.390842d*E. V0342 Aql |Halpha emission observed at Max light [08074]. The shape V0342 Aql |of the light curve and d apparently vary. Delta(m) V0342 Aql |probably decreases [08075]. V0343 Aql |Min II 10.7. V0346 Aql |Min II 9.1. ADS 13438 A (B 11.3m, 2", 245deg). V0346 Aql |Elements in the Table are valid after V0346 Aql |JD2437000. The shape of Min I varies [07001]. V0348 Aql |d ~0.08P. V0352 Aql |The nucleus of the supposed planetary nebula P.K. V0352 Aql |37-3.3deg. V0356 Aql |VB A (B 0.2"). V0367 Aql |The elements are satisfactory V0367 Aql |only during JD2436450 - 37960. Resembles S Vul. V0368 Aql |VB A (B 0.17", 140deg). V0374 Aql |VB A (B ~0.2', ~270deg). V0406 Aql |Min II 13.3:. V0407 Aql |P var; there is a nonlinear term in the elements: V0407 Aql |+1.51d*10**(-9)*E**2. V0409 Aql |Min II 12.2. Spectral type from another publication V0409 Aql |is A2 - A3. V0411 Aql |Epoch of Min is given. V0417 Aql |Min II 11.5. P var. Before JD2439000: V0417 Aql |Min = 2428427.127 + 0.3701251d*E. V0421 Aql |P var? V0423 Aql |Elements are valid for JD2426900 - 28000. During V0423 Aql |JD2429020 - 31670 the waves are much longer or absent. V0433 Aql |Waves of 26d - 80d duration with Delta(m) = 0.1m - 0.9m. V0433 Aql |The mean light varies according to the formula V0433 Aql |Max = 2438312 + 648d*E. V0449 Aql |The star in [01091,02282] is actually not identical to HV5424. V0461 Aql |Close component ~15.5m, the range of combined light is V0461 Aql |given. V0467 Aql |Waves of 40d - 72d duration. The mean light varies with V0467 Aql |P ~1400d. V0473 Aql |P ~330d is sometimes observed. V0476 Aql |EW type with doubled period is possible. Elements are based V0476 Aql |on a short series of observations. V0483 Aql |In the field of the open cluster NGC 6709. V0486 Aql |In the field of the open cluster NGC 6709. V0493 Aql |B - V: +1.10, +1.38. V0495 Aql |d = 0.06P:. V0496 Aql |B - V: +1.07, +1.28. Elements are given for epochs after V0496 Aql |JD2428000. V0497 Aql |VB A (B 16.5m, 9", ~0deg). V0524 Aql |The variable is np from the star shown in the chart V0524 Aql |in [02317]. V0527 Aql |IS type is possible. V0528 Aql |VB A (B 16.5m, 11", 59deg). V0535 Aql |VB [01943], two components are seen on Palomar prints, V0535 Aql |eastern of them being red. According to [01943], rapid V0535 Aql |variable. V0537 Aql |Possible P = 200d. V0538 Aql |Possible P = 375d. V0558 Aql |Possible P = 187d. V0571 Aql |Possible P = 185.5d. V0572 Aql |B - V: +0.65, +0.87. P var. Before JD2435500 P ~3.7686d. V0572 Aql |See also [08637]. JD2433631.8421 + 0.716292d*E. V0572 Aql |See also [02124]. V0586 Aql |Irregularities are sometimes observed, but then the V0586 Aql |periodicity is probably resumed. V0596 Aql |Resembles S Vul. V0599 Aql |Min II 6.73. According to [08083], may be constant. V0600 Aql |B - V: +1.36, +1.70. V0600 Aql |Before JD2428000 another value of P is possible [08632]. V0602 Aql |d = 0.02P. Min II 12.7. V0603 Aql |SB (P = 0.13854d [03169]). Outside the outburst there are V0603 Aql |variations of light (eclipses) with Delta(m) = 0.30m, V0603 Aql |Min I = 2444401.399 + 0.1377d*E (D ~0.2P). The V0603 Aql |shape of the light curve and the depth of minima differ V0603 Aql |from cycle to cycle. The brightness in minima shows V0603 Aql |fluctuations apparently connected with the presence of V0603 Aql |a hot spot [04500]. V0605 Aql |A unigue variable. 8" np from a 17m star. Min ~20m pg. V0605 Aql |Photographs of the field [06041,06042]. The V0605 Aql |light curve resembles those of the SN in NGC V0605 Aql |1058 or of eta Car [06040]. The only Max observed, with V0605 Aql |fluctuations, occured in 1918 - 1924. In 1921 the spectral V0605 Aql |type was found to be R [02464]. The star is inside the old V0605 Aql |planetary nebula A 58 and may be its nucleus. V0609 Aql |Min II 11.9. V0615 Aql |P var? Max = 2428046 + 364d*E (JD2428038 - 31343) [01091]. V0616 Aql |d = 0.04P. Elements reguire verification. V0618 Aql |Twice shorter period is not excluded. V0637 Aql |Twice shorter period is not excluded. V0638 Aql |Twice shorter period is not excluded. V0640 Aql |Min II 12.8. V0647 Aql |Slight Min II [01091]. V0663 Aql |P = 194.5d is possible. V0666 Aql |The range is given for combined magnitude with a preceding V0666 Aql |16.5m star. Separately was found ~17m pg near Min. V0672 Aql |P var? Blazhko effect is possible [03113]. V0678 Aql |P var. Before JD2429723 Max = 2429723 + 120.6d*E. V0688 Aql |Min II 10.8. DII = 0.15P. V0694 Aql |d = 0.13P. VB (1"), a companion ~1m fainter than V0694 Aql |the variable [01881] may have affected the data given. V0699 Aql |Min II 13.75. V0706 Aql |Delta(S) = 0:. V0708 Aql |P ~65d waves superimposed on slow variation of mean V0708 Aql |brightness with P ~1350d (JD2437124 - 40512) [06025]. V0708 Aql |According to [00773] waves with P ~100d - 150d V0708 Aql |(JD2427543 - 31318). V0714 Aql |d = 0.05P. V0724 Aql |Min II 11.57. V0733 Aql |P var? Before JD2434500, V0733 Aql |possibly Max = 2434453.72 + 6.17687d*E [00001]. V0734 Aql |VB A? (B 16.1m?). V0743 Aql |White. SRD? V0755 Aql |Alternative elements: Min = 2429195.290 + 1.01598d*E. V0765 Aql |B - V: +0.70, +0.80. V0766 Aql |EW type is not excluded. V0769 Aql |d = 0.05P? V0770 Aql |Min II 14.0. V0771 Aql |According to [03165] UG. V0774 Aql |Possibly resembles UV Boo. V0777 Aql |P = 111.5d is possible. V0784 Aql |Min II 14.8. V0794 Aql |Rapid changes with Delta(m) up to 1.5m superimposed on V0794 Aql |slow ones. May belong to "polars" of XPRM type. Peculiar V0794 Aql |spectrum with broad emissions and blue continuum [08676]. V0800 Aql |VB. According to [06072] UGZ. V0801 Aql |VB A (B 15.1m sp). V0803 Aql |Min II 14.8. V0804 Aql |Min II 12.8. In Max B - V = +0.61. V0805 Aql |Min II 7.90, DII = 0.11P. V0808 Aql |Min II 13.3. V0812 Aql |VB A (B 16m sp, C 16m sf). V0814 Aql |VB A (B 16.5m sp). V0822 Aql |Min II 7.07. ADS 12538 A (B 10.1m, 1", 67deg). The shape V0822 Aql |of the light curve varies.(U - B) index in Min I is redder V0822 Aql |and Min II is bluer than average. V0829 Aql |Twice longer P is possible. V0836 Aql |RR type is possible ([00085]; it is suggested also by the V0836 Aql |spectrum [08676]). V0850 Aql |In the centre of the planetary nebula P.K. 37-6.2. V0866 Aql |Min II 14.8. According to [06026], the depth V0866 Aql |of Min II 0.4m, EB type. V0867 Aql |P var? V0871 Aql |Min II 14.5, Min II - Min I = 0.425P. V0871 Aql |Physical changes in the range 13.3 - 13.6 are V0871 Aql |possible. Eclipses start from the 13.6m level. V0872 Aql |Min II 15.7:. Apsidal motion is possible. V0873 Aql |P var? The mean light varies in the range 13.8 - 14.0. V0875 Aql |White. According to [06004], rapid. Possibly UGZ or IA. V0877 Aql |VB A (B 16.5m nf). V0882 Aql |Blazhko effect is possible. V0885 Aql |Min II 14.9:. Apsidal motion and changes of the shape of V0885 Aql |the light curve are possible. V0888 Aql |A possible member of the open cluster NGC 6738. V0889 Aql |Min II 9.0. Min II - Min I = 0.35P. V0889 Aql |Apsidal motion is possible. V0890 Aql |Nova Aql 1946 = asteroid N258 Tyche [09038]. V0891 Aql |Min II 15.8. V0895 Aql |P var. Max = 2430931.435 + 0.265108d*E V0895 Aql |(JD2426920 - 35010) [02267]. V0895 Aql |During JD2441890 - 42290 - see Table. V0907 Aql |Min II 15.7. V0912 Aql |The shape of the light curve varies. V0914 Aql |P = 3.336217d V0914 Aql |is given in [08717] by misprint. V0919 Aql |Min II 13.8. V0920 Aql |F or earlier observations Max = 2429458.400 + 0.4955033d*E. V0922 Aql |Elements are not quite reliable. V0923 Aql |Unusual shell star [01884]. Similar to EW Lac. V0923 Aql |He lines are widened by the rotation, NaI lines V0923 Aql |are narrow. Light changes are periodic: Min = V0923 Aql |2436458.66 + 0.8518d*E. The cause of variations is V0923 Aql |probably connected with the rotation and the inhomogeneous V0923 Aql |brightness distribution over the disk of the star [03178]. V0923 Aql |Profiles of spectral lines vary. The expansion of the V0923 Aql |envelope terminated in 1965, which apparently led to the V0923 Aql |development of inhomogeneities and to the broadening of V0923 Aql |hydrogen line profiles [04525]. V0925 Aql |Some observers found constant brightness [03165]. V0929 Aql |Short period. V0936 Aql |Short period. V0947 Aql |According to [05412], rapid irregular V0947 Aql |changes are not excluded. According to [00504], constant. V0955 Aql |Min II 14.9, DII = 0.13P. V0956 Aql |Min II 14.2. Elements need confirmation. V0957 Aql |P var. Max = 2428154.960 + 0.6051327d*E V0957 Aql |(JD2421871 - 28105). V0958 Aql |VB A (B 17.0m, 0.2' np; C slightly brighter, 0.1'f). V0958 Aql |Combined magnitude of A and C is given. V0964 Aql |Min II 13.7. V0969 Aql |Blazhko effect is possible. V0981 Aql |Min II 14.5. V0991 Aql |IS type is possible. V0992 Aql |According to [04260], P = 110d. V0998 Aql |The position coincides with the planetary nebula V0998 Aql |P.K.50-3.1deg. V0999 Aql |Tsessevich's observations [07806] do not agree with the V0999 Aql |elements in the Table. V1017 Aql |Elements need confirmation. V1033 Aql |P var? V1045 Aql |Min II 13.5. V1046 Aql |P var? [08321].Min = 2427713.314 + 5.28303d*E [04027]. V1046 Aql |Slight reflection effect is possible. V1064 Aql |Cycles 295d - 410d. V1072 Aql |sp component of a close pair. V1075 Aql |d = 0.04P. Min II 13.6. V1076 Aql |VB A (close preceding). V1086 Aql |VB. Probably the variable is the sf component. V1093 Aql |IA type is possible. V1095 Aql |P var. After JD2429048 - see Table, earlier V1095 Aql |Max = 2427322 + 42.68d*E. Not coloured appreciably. V1096 Aql |Min II 13.3. V1097 Aql |Min II 14.0. V1101 Aql |Possibly UGZ type [03156]. V1113 Aql |The period may be twice shorter. V1117 Aql |Min II 16.6. V1125 Aql |Min II 16.0. V1140 Aql |P var? V1154 Aql |Min II 14.8; Min II - Min I = 0.70P. V1165 Aql |According to [04564], constant. In [03932] was not separated V1165 Aql |from a close component which probably led to distortions V1165 Aql |of the light curve. V1166 Aql |UG type is possible. V1173 Aql |nf component of a close pair. V1182 Aql |Min II 8.65. V1184 Aql |Min II 13.4. V1200 Aql |VB. The variable is the eastern red component. V1204 Aql |VB. The variable is the eastern component. V1208 Aql |A common proper motion star 9.06m in 1' to the south. V1248 Aql |UG type is possible. V1251 Aql |Red. V1261 Aql |Spectral type K2 in HD. V1269 Aql |VB. The variable is the preceding component. V1281 Aql |Reddish. SRD type is possible. V1286 Aql |Possibly the period is accidental. V1288 Aql |ADS 12182 A (B 12.3m, 36", 287deg). V1291 Aql |The elements have been determined on the base of magnetic V1291 Aql |field variations. The epoch of minimum intensity of the V1291 Aql |magnetic field is given. V1295 Aql |Shell star. Dramatic spectral changes were observed [05240]. V1295 Aql |The variability is hardly periodic, though P ~100d is V1295 Aql |possible. Sometimes light fluctuations on several days' V1295 Aql |time scale are observed [05880]. IR excess [06277]. For a V1295 Aql |detailed spectroscoric study, with evidence for the V1295 Aql |outflow of matter from the surface, see [04739]. V1295 Aql |Considerable magnetic field [04435]. V1297 Aql |d = 0.05P? Min II 14.5. V1298 Aql |mu alpha = -0.0392s, mu delta = -1".330. V1298 Aql |The companion of the star BD +4deg 4048 (ro = V1298 Aql |73".8, theta = 151.5 deg). V1298 Aql |One of the absolutely faintest known stars (Mv = +19m). V1300 Aql |I - K: +5.2, +6.5. Sometimes CO, SiO, OH maser emission. V1302 Aql |A unique IR object IRC +10420. B - V = +2.7, U - B = +1.9. V1302 Aql |OH, H2O, SiO maser. According to [07437], the energy V1302 Aql |distribution in the IR spectrum (1 - 22mkm) resembles that V1302 Aql |of eta Car. Emissions of neutral metals are observed in V1302 Aql |the spectrum. Increased in brightness during 1925 - 1970; V1302 Aql |Max ~1970. V1323 Aql |Close VB; var - northern component. V1325 Aql |VB, np component var. V1331 Aql |Min II 7.95. According to [04619] P = 1.364076d. V1333 Aql |Aql X-1. Light variations with P ~1.28d - 1.31d due to V1333 Aql |orbital motion are possible [04625]. Bursts characteristic V1333 Aql |of the XB type are observed [04757]. Lx/Lopt ~500 outside V1333 Aql |nova-like bursts, Lx/Lopt ~5000 during bursts. V1336 Aql |In 1.6' W from MXB 1916-05. M type is possible. V1338 Aql |VB. Probably the f component, very bright infrared, is var. V1340 Aql |d = 0.06P? Intrinsic lightvariations in Max are possible. V1341 Aql |Min II 13.4. P = 0.3586768D is possible. V1343 Aql |SS 433. <B - V> = +2.0. Associated with the SNR W 50. Mean V1343 Aql |light varies in the range 14.0 - 14.6 V according to the V1343 Aql |elements Max = 2443662.5 + 165.5d*E [00512]. The depth of V1343 Aql |Min I varies from 0.2m to 0.9m V, the depth of Min II V1343 Aql |varies from 0 to 0.4m V. Two systems of H, HeI, HeII V1343 Aql |emission lines are observed in the spectrum: the V1343 Aql |"stationary" system corresponding to Vr changes from 300 V1343 Aql |to 150 km/s with P = 13.1d, and the "relativistic" one, V1343 Aql |corresponding to Vr changes from +50000 to -35000 km/s V1343 Aql |with P = 165.5d. The spectral study [00535]. The system V1343 Aql |apparently consists of an O - B star filling its inner V1343 Aql |Roche lobe and a compact object surrounded by an accretion V1343 Aql |disc wich is precessing with P = 165.5d. Two jets V1343 Aql |consisting of dense condensations of matter emerge from V1343 Aql |the system with relativistic velocity (0.27 c) in opposite V1343 Aql |directions. The luminosity of the disc amounts to not less V1343 Aql |than 60% of the total luminosity of the system [00926,00953]. V1343 Aql |The object may be a former supernova which bursted not V1343 Aql |more than 10**4 years ago. V1345 Aql |Min II 14.3:, Min II - Min I = 0.46P. V1349 Aql |Max ~17 pg. V1352 Aql |VB A (B 14.5m, 6", 175deg). V1353 Aql |Min II 10.9. V1355 Aql |Min II 13.3. V1357 Aql |Possibly P = 1.051d. V1470 Aql |The variability may be due to the fainter (B) component. V1472 Aql |SB, Porb = 198d. V1648 Aql |Brightening over 10 years, probably due to dissipating dust envelope, V1648 Aql |plus quasi-periodic variations. eta Aql |P var. P = 7.176344d (JD2373000 - 95100), eta Aql |P = 7.176455D (JD2395100 - 2412100). Since JD2412100 - eta Aql |see Table. For the whole interval eta Aql |Max = 2442794.773 + 7.176735d*E + 2.18d*10**(-8)*E**2 eta Aql |[08632]. In the UV band the light of a possible A0V eta Aql |comparion is apparent. sig Aql |ADS 12737 A (B 12.34m, 48", 328deg). Depth of Min II 0.1m. sig Aql |In [04627] P = 1.950271d is given according to sig Aql |spectroscopic data. R Ara |Min II 6.2. VB A (B 8.2mV, 4", 123deg). S Ara |(k - b)2 = 0.09. P var [01932,03126]. Max = 2416284.792 + S Ara |0.45188910d*E (JD2414000 - 19000);Max = S Ara |2419149.797 + 0.45188581d*E (JD2419000 - S Ara |30000) [00752]. Since JD2441000 - see Table. For the S Ara |whole interval, with sufficient accuracy, S Ara |Max = 2420047.2382 + 0.451888176d*E - 1.36d*10**(-10)*E**2 S Ara |[03126]. T Ara |VB A (B 11.0m, 34", 60deg). X Ara |Shown in the chart for S5809. RT Ara |According to Cannon [01944] who discovered the star's RT Ara |variability, a companion 12.0m is present in 0.1m to W RT Ara |and somewhat to the north from the variable. Cannon points RT Ara |out that at Min light the variable becomes fainter than RT Ara |the companion. No sign of the companion's existence was RT Ara |found by Hoffmeister [00016] and by Payne-Gaposchkin [00624]. RT Ara |According to [00624], the mean cycle is ~78d, and RVA RT Ara |type is possible. RW Ara |d = 0.022P. Min II 8.91. Changes of the shape of the light RW Ara |curve due to gaseous streams or a hot spot are possible. TT Ara |ZrO bands may be present in the spectrum [03181]. TV Ara |In the region of the cluster NGC 6208. TX Ara |VB A (B 16.5m). Twice shorter period is possible. XX Ara |Min II 14.1. YY Ara |The star's being an eclipsing or irregular variable is not YY Ara |excluded [00424]. AA Ara |Min II 13.3. AD Ara |[A/H] = -0.4. AE Ara |VB A (B 12m, 0.3' sf). P.K. 344-8.1. AE Ara |A compast planetary nebula or a symbiotic star. Irregular AE Ara |abrupt brightenings by 3m - 4m separated by several years AE Ara |are observed [00255]. The spectral data are discussed in AE Ara |[08076]. AF Ara |Min II 13.8. AW Ara |Before JD2417300 Max = 2412600 + 186d*E. BQ Ara |Double maxima separated by 10d - 20d, with Min II 12.8. CC Ara |VB; the variable is nf component. CH Ara |Noted on the finding chart for S6062 = V 466 Ara. CT Ara |Before JD2420400 Max = 2413080 + 215d:*E; CT Ara |since JD2425000 - see Table. DU Ara |B - V: +0.52, +0.84. P var. Max = 2418145.560 + DU Ara |1.63999d*E (JD2411000 - 21000); Since DU Ara |JD2425000 - see Table. EK Ara |VB A (B 15m). EL Ara |Before JD2420400 Max = 2415140 + 332d*E; EL Ara |since JD2425000 - see Table. ER Ara |Min II 14.2. EV Ara |Before JD2420400 Max = 2413750 + 237d*E; EV Ara |since JD2425000 - see Table. EZ Ara |P var. FU Ara |The depth of Min I is 0.97m and 0.89m, FU Ara |the depth of Min II is 0.20m and 0.23m in blue and FU Ara |yellow light, respectively. GK Ara |Before JD2417800 Max = 2414050 + 237d*E, GK Ara |since JD2418400 - see Table. GM Ara |Min II 12.8. HX Ara |B - V: +0.23, +0.36. A hump on the ascending branch HX Ara |(phi = 0.93P) [08118]. KY Ara |Only one sharp Max (JD2428715 - 712) was observed. KY Ara |Possibly a Nova. KZ Ara |VB A (B 14.1m sp). LP Ara |d = 0.04P? Min II 10.5? LQ Ara |In 1959 rapid variations at times for 0.5m near 11m LQ Ara |were observed; surrounded by a nebula [04001]. LR Ara |Min II 10.6. LU Ara |Min II 10.1? MQ Ara |nf component is variable. MR Ara |B - V: +0.72, +0.8. [A/H] = -1.0. P var? QR Ara |Shown in the charp for BV 1443. QU Ara |VB. QW Ara |The variable is np component of the pair. QX Ara |Shown in the chart for S5818. V0340 Ara |B - V: +1.25, +1.68. [A/H] = 0.6. V0341 Ara |The star is blue; light variations during 4d were not V0341 Ara |accompanied by colour changes. Possibly an eclipsing V0341 Ara |variable [04678]. V0342 Ara |P >= 140d. V0344 Ara |P >= 170d V0345 Ara |P >= 180d. V0349 Ara |Min II 8.8. V0355 Ara |P > 220d. V0356 Ara |P > 170d. V0357 Ara |P >= 220d. V0360 Ara |Min II 13.8:, Min II - Min I = 0.35P. V0361 Ara |Min II 13.6:. V0362 Ara |Min II 15.6:. V0383 Ara |A star 16.5m is close to the north. V0421 Ara |Min II 15.1. V0440 Ara |Min II 14.5:. V0444 Ara |Min II 14.2. V0454 Ara |Min II 14.1. V0480 Ara |Min II 15.5:. V0484 Ara |RV type is possible (Min = JD2436760). V0485 Ara |Min II 14.8. V0489 Ara |Min II 11.9. V0491 Ara |Min II 11.9. V0492 Ara |Min II 14.5. V0494 Ara |RV type is not excluded. V0501 Ara |Min II 13.8. Shown in the chart for S6114. V0535 Ara |Min II 7.71. Nonlinear term in the elements: V0535 Ara |-4.4d*10**(-11)*E**2. V0536 Ara |Min II is present. EB type is possible. P var. V0536 Ara |P = 2.374101d (JD2415000 - 22000); since JD2422000 - V0536 Ara |see Table. V0539 Ara |VB A (B 9.22m, 12", 269deg). Min II 6.09, d = 0.01P. V0539 Ara |Shown in the chart for BV1441 = V538 Ara. V0544 Ara |14.5m star sp. V0609 Ara |Shown in the chart for S5867. V0610 Ara |EA type is possible. V0613 Ara |VB (close np companion is NSV10198). V0616 Ara |Deep Min II. V0620 Ara |Min II is possibly present. V0623 Ara |Min II 14.5. Twice shorter period is possible. V0624 Ara |P >= 220d. V0625 Ara |P >= 170d. V0639 Ara |V1 (NGC 6397). Probably not a cluster member. V0651 Ara |Min II 15.3. V0653 Ara |Min II 12.6. V0656 Ara |EW type is not excluded. V0658 Ara |Min II 16.0. V0659 Ara |Min II 14.4. V0668 Ara |Min II 13.8:. V0675 Ara |P >= 200d. V0687 Ara |RRC type is possible. V0700 Ara |Min II 15.7. V0702 Ara |Min II 14.0. V0704 Ara |Min II 13.3. V0705 Ara |Min II 14.4. RR type is possible. V0716 Ara |Monotonous brightening during JD2436689 - 36838 was V0716 Ara |found. The amplitude is probably greater. V0722 Ara |Min II 10.3:. V0728 Ara |Min II 12.8. V0732 Ara |CEP type is not excluded. V0743 Ara |RV type is possible. V0781 Ara |Min II 14.8:. V0783 Ara |Min II 13.9:. V0785 Ara |Min II 14.3. V0787 Ara |RV type is possible. Min JD2436756. V0789 Ara |Min II 14.8. V0790 Ara |Min II 14.8. V0791 Ara |Min II 13.0:. V0792 Ara |Min II 15.2:. V0801 Ara |MXB 1636-53. Description of the spectrum [01356]. V0801 Ara |Modulation with P ~4h and the amplitude up to 40% was V0801 Ara |found in the broad band optical flux [04944]. V0802 Ara |14.93 - 17.03 B. V0808 Ara |EW type is possible. V0820 Ara |Epoch of Min is given. Strong magnetic field. Either an V0820 Ara |eclipsing binary or (more probably) an object similar to V0820 Ara |rotating variables of ACV type. V0821 Ara |4U 1658-48. Unusua1 X-ray system. Quasiperiodic optical V0821 Ara |variations (P ~20s) with total amplitude 40 percent, V0821 Ara |abrupt bursts on ~20 ms time scale leading to two-fold V0821 Ara |flux increase and light changes by 6m during less than V0821 Ara |two months were observed [04958]. Lx/Lopt = 3. V0870 Ara |Type DSCT: is also possible. R Ari |OH emission. T Ari |P var. Max = 2417160 + 313.5d*E (JD2404800 - T Ari |17200); Max = 2434616 + 323.1d*E (JD2419400 - T Ari |34560). Since JD2436560 - see Table. <P> = 319.53d T Ari |(JD2404800 - 44160). Sometimes A < 1.5m. U Ari |SiO maser. V Ari |Vr = - 180 km/s. W Ari |Maps given in [02544,06067] are wrong. X Ari |B - V: +0.28, +0.56. P var. Max = 2420785.635 + X Ari |0.6511248d*E (JD2420460 - 33210) [03506]. Since X Ari |JD2433210 - see Table. [Fe/H] = -2.17. RR Ari |Min II 6.75:; Min II - Min I = 0.55P. Variability is not RR Ari |confirmed by other authors' photoelectric observations. RR Ari |V = 5.75. RS Ari |Min II 11.0. RU Ari |OH emission. RV Ari |B - V: +0.29, +0.44. 0.34P =< M - m =< 0.53P. RV Ari |P1 = 0.07195d [08137]; P2 = 0.27554d [07033]. Moments of RV Ari |brightest light maxima T = 2435066.400 + 0.31632996d*n RV Ari |[02290]. RW Ari |B - V: +0.35, +0.46. P var. Max = 2428183.324 + RW Ari |0.3543184d*E (JD2428040 - 36700) [03188]. Since RW Ari |JD2440900 - see Table. According to [06043] - EA type: RW Ari |Min I = 2439384.97 + 3.1754d*E. Total light range RW Ari |(11.47 - 13.25 V) [08127] seems doubtful. It is not RW Ari |excluded that the eclipses and light increase of RW Ari RW Ari |given in [08127] are explained by variability of one of RW Ari |comparison stars used. RX Ari |d = 0.02P. Depth of Min II 0.10m. SS Ari |P var. Min II 10.82:. ST Ari |P var. Max = 2427347 + 94.2d*E (1933 - 1939); Max = ST Ari |2429525 + 106.6d*E (1939 - 1942); Max = 2430588 + ST Ari |95.2d*E (1942 - 1946); Max = 2432118 + 100.0d*E ST Ari |(1946 - 1961). Mean elements are given in the Table. SX Ari |B - V: -0.10, -0.12. Epoch of Min is given. SZ Ari |d = 0.03P. TT Ari |Porb = 0.137551d [08138]. Along with light variations TT Ari |typical for Z Cam variables there are sinusoidal variations TT Ari |with amplitude of about 0.2m B and variable period: TT Ari |P = 0.1329d (1961 - 62), P = 0.1327d (1966) [04931], TT Ari |P = 0.1326d (1978) [04935]. Sinusoidal variations are TT Ari |superimposed by quasiperiodic oscillations up to 0.2m with TT Ari |8 - 20 minutes cycle and irregular flickering up to 0.1m TT Ari |in 1 minute. TU Ari |P var. Max = 2420463.353 + 0.4716219d*E TU Ari |(JD2420463 - 34720). Since JD2436820 - see Table. TV Ari |P var. TX Ari |P var? TY Ari |Form of the light curve varies. Mean value of the period TY Ari |is given. UV Ari |The second overtone period given in the UV Ari |Table is dominating. Sometimes the fundamental UV Ari |period P0 = 0.062d and the first overtone period P1 = UV Ari |0.047d are observed. UW Ari |Amplitude varies. In the interval JD2441581 - 693 - const. UW Ari |[07544]. UX Ari |T = 2440133.766 + 6.43791d*E [06444], where T is epoch of UX Ari |conjunction (G5 component is behind K0 component). UX Ari |Brightness varies in waves with a period ~Porb, but the UX Ari |phase psi of light minimum calculated according to the UX Ari |elements given above changes with time: psi = 0.1P UX Ari |(1972 - 1974), psi = 0.8P (1976), psi = 0.7P (1977), UX Ari |psi = 0.6P (1978). Mean brightness varies, amplitude of UX Ari |the wave varies from 0.04m up to 0.15m. VW Ari |BDS 1269 A (B 8.33m, 74", 31deg). P2 = 0.089d. VW Ari |Metal deficiency. The companion has normal metal abundance. VY Ari |SB? Epoch of Min is given. VY Ari |Second light variation is also observed: Min = VY Ari |2442044.6 + 43.9d*E. A small flare in U band was VY Ari |observed. gam Ari |VB A (B 4.65m, B 9 V, 7.9", 0deg). Epoch of Min is given. R Aur |VB A (B 8.6m, 48", 239deg). P var [07165]; R Aur |cycle 64.5a is possible. S Aur |P var. In the early fourties of our century the star was S Aur |faint with small and irregular variations. T Aur |Min = 2437614.0088 + 0.20437851d*E [08145]. P var? T Aur |<V> = 14.92, <B - V> = + 0.28. There are light T Aur |fluctuations between the eclipses. Depths of Min are T Aur |0.10m - 0.28m [03195]. Faint nebula with high degree of T Aur |ionization. U Aur |H2O maser. Y Aur |B - V: +0.70, +1.06. Z Aur |P var [07110]. Max = 2425580 + 110.76d*E Z Aur |(JD2416156 - 25580); Max = 2429888 + 113.35d*E Z Aur |(JD2425570 - 29900); Max = 2438292 + 135.55d*E Z Aur |(JD2429900 - 33300). P = 110d (1965) [03196]. Z Aur |In 1970 - irregular variations [07338]. <V> = -165 km/s; Z Aur |According to TiO bands the spectrum is M1 [00806]. RS Aur |P var. RT Aur |B - V: +0.39, +0.80. [A/H] = 0.1. P var. Max = RT Aur |2433040.867 + 3.728365d*E (JD2417970 - 33100). RT Aur |Since JD2433100 - see Table. Delta(V) var? RU Aur |OH emission. RU Aur |Mean magnitude probably varies with Pi = 10400d [01059]. RW Aur |VB A (B 12.5m, dM0e, 1.2", 254deg). RW Aur |The companion probably flares with an amplitude RW Aur |0.5m - 0.7m [03197,03198]. Possible period of axial RW Aur |rotation is 100d [07067]. OH emission. RX Aur |B - V: +0.76, +1.18; [A/H] = -0.1, P var? RX Aur |Nonlinear term: -0.70d*10**(-6)E**2? RZ Aur |P var. Min = 2422616.498 + 3.010593d*E RZ Aur |(JD2418000 - 26000); since JD2426000 - see Table. SS Aur |SB (P = 0.1805939d [06103]). SS Aur |Sometimes abnormal behaviour of the star is SS Aur |being observed when comparatively numerous and SS Aur |small light maxima arise. According to [08151] the SS Aur |mean cycle is 51.2d. SU Aur |Common proper motion with AB Aur (P = 3'). Associated SU Aur |with a small bright nebula. OH emission. SX Aur |Min II 8.87. According to [08153] P var: SX Aur |Min I = 2418218.7779 + 1.21007653d*E + 0.91d*10**(-10)*E**2. SY Aur |B - V: +0.92, +1.23. [A/H] = - 0.3. P var [05661]. SY Aur |Max = 2436853.57 + 10.144330d*E (JD2417900 - SY Aur |32380). Since JD2432380 - see Table. TT Aur |Min II 9.0. TV Aur |S5/6-. TW Aur |Mean magnitude varies with P = 1370d. TZ Aur |B - V: +0.08, +0.48. Delta(S) = 2. UU Aur |VB A (B 11m, 18", 222deg). UV Aur |VB A (B 10.96m, B 9 V, 3.4", 4deg). UV Aur |Bright lines [NeIII] and [OIII] in spectrum. UW Aur |Epoch of Min is given. UY Aur |VB A (B 12m?, 0.8", 212deg). OH emission. VW Aur |VB (9.0m, 11.8m, 1.4", 332deg, 1976). VX Aur |P var? WW Aur |Min II 6.43. Min II - Min I = 0.50P. XX Aur |Min II 13.4. YZ Aur |B - V: +1.15, +1.72. [A/H] = -0.4. ZZ Aur |Min II 11.1. AB Aur |Common proper motion with AB Aur (P = 3'). Associated AB Aur |with a small bright nebula. OH emission. Spectrum AB Aur |description [04002]. AE Aur |Connected with the bright nebula IC AE Aur |405. The motion is directed away from Ori OB 1 AE Aur |association with the velocity 106 km/s. AG Aur |According to TiO bands AG Aur |the spectrum is M3 [00806]. AH Aur |Min II 10.70. P var. AK Aur |VB B (A = BD +31deg 1370, 8.3m; B 82", 26deg). B - V: AK Aur |+0.18. AM Aur |Min II 11.0. P var: Min I = 2417617.2 + 13.6182d*E AM Aur |(JD2413500 - 19500) [00608]; since JD2425400 - see Table. AN Aur |B - V: +1.06, +1.48. [A/H] = -0.2. AO Aur |B - V: +0.86, +1.27. AP Aur |Min II 11.2. P var: Min I = 2423080.505 + 0.5692965d*E AP Aur |(JD2423080 - 35000). Since JD2435000 - see Table. AQ Aur |Light curve shape var? AR Aur |Min II 6.70. Min II - Min I = 0.50004P. P var: Min I = AR Aur |2427887.7217 + 4.13467d*E (JD2427800 - 29500) [04999]. AR Aur |Since JD2438400 - elements in the Table with an additional AR Aur |nonlinear term: -2.2d*10**(-8)*E**2. AZ Aur |Close companion 16.3m B. BC Aur |Min II 11.7. BF Aur |Min II 9.49. P var. Min I = 2434455.3872 + BF Aur |1.583217d*E (JD2411760 - 34455) [05038]. Since JD2434455 BF Aur |- see Table. The two sets of observations are equally well BF Aur |represented by the formula: Min I = BF Aur |2440628.3643 + 1.5832212d*E + 1.7d*10**(-10)*E**2 [08160]. BH Aur |P var. Max = 2437352.461 + 0.45608821d*E (JD2417260 - BH Aur |42750) [07806]. Since JD2442750 - see Table. BK Aur |B - V: +0.86, +1.26. CI Aur |Depth of Min II 0.05m. P var. Min I = CI Aur |2439414.573 + 1.869984d*E + 0.020d*10**(-8)*E**2 CI Aur |(JD2425560 - 42045). Elements given in the Table represent CI Aur |observations in the interval JD2439052 - 40654. CL Aur |Min II 12.3; Min II - Min I = 0.45P; DII = 0.13P. P var? CL Aur |Min I = 2432967.262 + 1.2443666d*E (JD2416900 - 32967) CL Aur |[00608]. Since JD2432967 - see Table. CO Aur |The first overtone period is CO Aur |given in the Table; the second overtone P = 1.4255d. CQ Aur |B - V: + 0.86, + 1.07; Min II 9.14:; Min II - Min I = CQ Aur |0.52P:; D = 0.096P. P var. Nonlinear term: CQ Aur | +3.78d*10**(-7)*E**2. CY Aur |[A/H] = -0.3. DV Aur |P var. Max = 2426015 + 198.0d*E (JD2426014 - 27400) [00332]. DV Aur |Since JD2439940 - see Table. EI Aur |Min II 15.0. EM Aur |Min II 11.7. EO Aur |Min II 7.89. EP Aur |Min II 10.9. P var? ER Aur |[A/H] = - 1.1. P var? Max = 2432951.54 + 15.69073d*E ER Aur |(1949 - 1950) [01059]. In the interval JD2443428 - 874 - ER Aur |see Table. EW Aur |[A/H] = - 0.6. FF Aur |[A/H] = - 0.3. FN Aur |Min II 12.3. P var? FP Aur |d = 0.080P. FR Aur |Min II 13.0. FZ Aur |d = 0.40d. GI Aur |Min II 11.7. GK Aur |Min II 14.0; Min II - Min I = 0.62P. GO Aur |P var. Max = 2426071 + 292.1d*E (JD2425505 - GO Aur |31325); Max = 2432205 + 301.2d*E (JD2432805 - GO Aur |36120) [03211]. Since JD2436990 - see Table. GY Aur |Min II 13.3. HL Aur |Min II 11.0. HN Aur |In the cluster NGC 1664. HN Aur |Light variations with P2 = 1400d: are HN Aur |superimposed by variations with P1 = 165d:. HP Aur |Min II 11.28; Min II - Min I = 0.502P. P var. Min I = HP Aur |2427445.400 + 1.4228180d*E (JD2427445 - 42683); since HP Aur |JD2442712 - see Table. HR Aur |Epoch of Min is given. HS Aur |Min II 11.2. The value of period given in [02619] must be HS Aur |doubled as the system consists of two equal components HS Aur |[08164]. HU Aur |Min II 12.4. HW Aur |Min II 12.6. HZ Aur |Sometimes short period variations of Vr with the amplitude HZ Aur |3 km/s and of brightness in U with the amplitude 0.02m are HZ Aur |also observed. Max Vr = 2439454.900 + 0.073502d*E HZ Aur |[05259]. P (DeltaU) = 0.07396d [04818]. II Aur |Min II 15.0:. IM Aur |Min II 8.05:. IQ Aur |Epoch of Min is given. IS Aur |VB. The range of combined brightness variation is given. IS Aur |It is not known which of the components varies. IU Aur |P var. There is an additional periodic term in the elements: IU Aur |-0.00627d*sin (2.221deg*E + 15deg). The ratio of Min II IU Aur |depth to Min I depth is 0.78. There is secular deepening IU Aur |of both minima. The depth of Min I increases by 0.016m per IU Aur |year. The range of light variation in the Table is given IU Aur |for 1979.0 (Min II 8.69). Orbital inclination is increasing IU Aur |by 0.5deg per year [05181] due to orbital precession caused IU Aur |by a third body. Spectrum description [08166]. KO Aur |Min II 11.2. KR Aur |<B - V> = +0.10, <U - B> = -0.95. SB (P = 0.1628d [09045]). KR Aur |Spectrum description [08169,08170]. Wide hydrogen emission KR Aur |lines. Long maxima and minima lasting for years are KR Aur |superimposed by rapid light variations by 1 - 2m in KR Aur |several days or fortnights and by 0.5m in dozens of KR Aur |seconds [08168,08170]. The source of soft X-rays [05191]. KS Aur |VB A (12.5m, 5", 94deg). KV Aur |Flat waves with a cycle about 750d are sometimes KV Aur |superimposed by comparatively rapid fluctuations. KW Aur |VB A (B 11.0m, 11.1", 352deg, 1909; C 7.99m, 14.5", KW Aur |226deg, 1923); SB1 (P = 3.788568d). Mean light level KW Aur |varies synchronously with orbital motion. Besides main KW Aur |pulsational period there are two more periods of nonradial KW Aur |pulsation: P1 = 0.096533d, P2 = 0.088243d. KX Aur |In the IC 405 nebula. KY Aur |In the IC 405 nebula. LY Aur |VB A (B 9.1m, 0.6", 249deg, 1958). Min II 7.26; d = 0.017P. MR Aur |Min II 15.5. MT Aur |d = 0.02P. NP Aur |P var. Since JD2437720 - see Table. NU Aur |Blazhko effect. Pi = 179d:. NV Aur |OH, SiO, H2O maser. NW Aur |In the region of the NGC 1893. Min II 14.7. NW Aur |According to [07160] no minimum was recorded during NW Aur |visual observations covering twice all phases. NX Aur |In the cluster NGC 1893. OP Aur |In the cluster Stock 8. OX Aur |VB A (B 10.0m, 22.4", 224deg). P1 = 0.115442d. OX Aur |Mean brightness probably varies. PR Aur |The chart in [07806] is wrong. PY Aur |Possibly a cepheid. QR Aur |Epoch of Min is given. QY Aur |SB. V0348 Aur |VB A (B 13.43m, 24", 44deg). V0353 Aur |During several decades the star brightened by 0.06m in a V0353 Aur |year. Possibly a planetary nebula in the process of V0353 Aur |formation. V0358 Aur |In the region of the cluster NGC 2099. V0411 Aur |The HD catalogue identifies HD 32447 with BD+30 775, wich V0411 Aur |is V0411 Aur. In the HDE Atlas V0411 Aur = HD 282867, and V0411 Aur |HD 32447 is a different star. V0431 Aur |P = 16.86d detected in HIPPARCOS data. V0433 Aur |SB? V0527 Aur |Also might be a low-amplitude Cepheid. bet Aur |VB A (B 14.1m, 13", 174deg). Min II 1.98. eps Aur |VB A (B 14.0m, 21", 224deg). d = 0.037P. eps Aur |Survey of the physical properties of the system [02041, eps Aur |02042, 03070, 03216, 03217, 08174]. The spectrum probably eps Aur |varies even outside eclipses. The eclipses are probably eps Aur |due to a disk of gas and dust surrounding the hot eps Aur |companion. The brightness has physical fluctuations eps Aur |with the amplitude up to 0.24m and the cycle about 110d eps Aur |[02040] which hinder revealing the possible Min II. eps Aur |Similar cycle was discovered also in the fluctuations eps Aur |of Vr. zet Aur |Range of light variation strongly depends on lambda: zet Aur |4.98 - 5.53 B, 5.36 - 7.33 U. d = 0.039P var: zet Aur |37.58d <= d <= 38.07d [05486]. Light fluctuations of zet Aur |K star by 0.05m [05539]. tet Aur |VB A (B 7.5m, 2", 8, 331deg, 1924). tet Aur |According to [04034] the period of magnetic field variation tet Aur |is 3.618d. U Boo |Delta(m) var (from 0.9m to 2.4m). V Boo |P var. Amplitude strongly varies. W Boo |According to [06994], P = 30d +-. Z Boo |H2O maser. RS Boo |Delta(S) = 2. P var. Before JD2435000 Max = RS Boo |2418115.5867 + 0.37733691d*E; since JD2435000 - see RS Boo |Table. Changes of the height of maxima: Max (minimal RS Boo |height) = JD2442500 + 533d*E; a shorter cycle of changes RS Boo |is possible: P ~ 58 - 62d [04832]. RU Boo |B - V: +0.09, +0.44. RX Boo |H2O, SiO, OH maser. SS Boo |Depth of Min II 0.1m. ST Boo |P var. Max = 2439236.032 + 0.6222968d*E (1966 - 1974). ST Boo |Mean elements 1911 - 1974 - see Table. Blazhko effect: Min ST Boo |(O - C) = 2442203 + 284d*n. Delta(S) = 11. SU Boo |D = 0.032P. Min II 12.04. P var. SV Boo |B - V: +0.17, +0.44. P var? SW Boo |B - V: +0.09, +0.39. P var. Before JD2426500 SW Boo |Max = 2421840.295 + 0.5134948d*E [02008,02011]. Since SW Boo |1960 - see Table. Secondary oscillation: Max (height of SW Boo |Max) = 2441037.33 + 12.997d*E. According to [04833], the SW Boo |magnitude in Max varies between 10.5 and 11.6 V. SZ Boo |P var? TU Boo |Min II 12.4. TV Boo |B - V: +0.10, +0.22. [Fe/H] = -2.42. TV Boo |Blazhko effect, Pi = 16.14d [07116]. TW Boo |B - V: +0.11, +0.40. Delta(S) = 12. P var. Before TW Boo |JD2426890 Max = 2420340.551 + 0.53227557d*E; TW Boo |since JD2426890 - see Table. TY Boo |Min II 11.35.P var. TZ Boo |Min II 10.82 (var). dII = 0.09P. P var. Depths of minima TZ Boo |vary from 10.8 to 11.0 V with P ~3.5 yrs; sometimes Min II TZ Boo |is deeper than Min I. Some other parameters of the shape TZ Boo |of light curve are also variable. In ~1960 the period TZ Boo |changed abruptly; other period variations were also noted. UU Boo |B - V: +0.03, +0.44. P var. Period change ~JD2432700 UU Boo |[03230]. Earlier Max = 2424967.310 + 0.45690626d*E [03229]. UW Boo |Min II 10.5. UX Boo |According to [02136], Delta(m) ~0.5m pg, EW? UY Boo |Delta(S) = 12.6. P, Delta(m) var. Before JD2425500 UY Boo |Max = 2411459.819 + 0.6508552d*E; Max = UY Boo |2425688.836 + 0.6507849d*E (JD2425500 - 28670) [01702]; UY Boo |Max = 2432306.759 + 0.650799d*E (JD2428670 - 32300) UY Boo |[02431]. Since JD2435900 - see Table. VW Boo |Min II 10.93. P var. Nonlinear term: VW Boo |-0.084d*10**(-9)*(E - 7500)**2. WY Boo |Possibly P = 90d. XY Boo |Min II 10.61. P var. YZ Boo |Delta(S) = 0. Delta(m) var, the shape of the light curve YZ Boo |varies [08186]. ZZ Boo |Min II 7.44. Possible radio source. AC Boo |Min II 10.55. P var? Depth of minima and level of maxima AC Boo |are variable. AD Boo |Min II 9.9. AE Boo |P var. (k - b)2 = 0.01. AG Boo |Blazhko effect is possible. AK Boo |Min II 16.3. AO Boo |P var. Mean period is given. AR Boo |Min II 14.5. P var. AS Boo |Blazhko effect is possible. BD Boo |Blazhko effect is possible. BE Boo |Scatter in the light curve near max light; BE Boo |P var? [05264]. The value of the period in the BE Boo |Table may be spurious. BG Boo |Min II 14.3. BI Boo |In the region of the globular cluster NGC 5466. BK Boo |Min II 15.3. BL Boo |V 19 (NGC 5466). B - V: +0.12, +0.25. [Fe/H] = -1.35. BL Boo |"Anomalous cepheid". Radial velocity cluster member. BN Boo |In the region of the cluster NGC 5466. BO Boo |The shape of the light curve varies: magnitude in BO Boo |Max - from 14.5 to 15.0. BP Boo |5.51 V. BR Boo |The mean light curve shows scatter which may evidence for BR Boo |the necessity to improve the period. BU Boo |P var. Mean period is given. AO Boo. The mean light curve BU Boo |could not be obtained. BW Boo |Min II 7.17. Min II - Min I = 0.450P. DII = 0.06P. SB1. BX Boo |VB A (B 10.6m, 36", 156deg). P var. According to other BX Boo |sources: Min = 244076730 + 0.741285d*E [07955]; BX Boo |Min = 2440767.26 + 0.6080722d*E [05054]. CC Boo |The star is not red. CD Boo |The star is not red. CK Boo |Min II 9.23. CP Boo |P > 0.125d. EL Boo |Type E: is also possible. gam Boo |VB A (B 12.5m, 33", 111deg, 1925). Delta(m) var. Radial gam Boo |velocity varies with P = 0.25d +-0.02d [04914]. kap 2 Boo |ADS 9173 A (B = kappa1 Boo, 6.69m, SB, F2V, 13",236deg). kap 2 Boo |According to [07015], P = 0.0668d. kap 2 Boo |Beat period ~16d [06086,07015]. ksi Boo |ADS 9413 AB (4.7m, G8V; 6.6m, K4V; A = 4.884", P = 149.95a). ksi Boo |LiI lambda 6708 line is present in the G8V spectrum. Both ksi Boo |spectra show manifestations of chromospheric activity, ksi Boo |emissions of H and K Ca II. Soft X-ray source. Probably it ksi Boo |is component A that is variable, though variability of H ksi Boo |and K CaII emission with the cycle 10 - 11 years ksi Boo |is observed for component B. i Boo |ADS 9494 B (A 5.1m, G0; a = 3.8", e = 0.43, P = i Boo |225a). Min II 6.29. P var. Min = 2434132.517 + i Boo |0.267812271d*E + 0.115242d*10**(-9)*E**2 (1916 - i Boo |1958) [03239]; Min = 2438513.4166 + 0.2678143d*E i Boo |(1947 - 1967) [08191]; since 1968 - see Table. Detailed i Boo |studies of period changes [05222,07352,07353,08181]. Sudden i Boo |period changes at JD2423800, 29300, 32300, 35150 are i Boo |possible. The shape of the light curve and the depth of i Boo |Min II are also variable. According to [02020], it is also i Boo |possible that ADS 9494 A is variable, with the amplitude i Boo |up to 0.09m. S Cae |<B - V> = +0.33. P < 1d. X Cae |(k - b)2 = 0.22. RX Cae |Variability type and spectral type (F3/F5II) do not agree. R Cam |S2/5:e. P var. T Cam |S5/5e. U Cam |Interfering P1 = 435.45d, P2 = 223.17d; P3 = 3000d [01053]. V Cam |H2O, SiO maser. Y Cam |EA/SD. SB1. Min II 10.60. P var. Min = Y Cam |2424434.5071 + 3.3054975d*E + 0.1215d* Y Cam |sin (0.0543deg*E + 186.8deg) (JD2411400 - 33300) [00978]; Y Cam |Min = 2437375.4923 + 3.3055069d*E + 5.3d*10**(-8)*E**2 Y Cam |(JD2437375 - 41000) [07166]; since JD2440000 - see Table. Y Cam |The primary component is a DSCTC variable [07166] with Y Cam |A <= 0.05m B. According to [04192], the pulsational period Y Cam |is possibly synchronized with the orbital motion and Y Cam |remains practically constant (0.066458d) during a long time Y Cam |interval. Z Cam |SB2. Lower conjunction of the G component Z Cam |T = 2438470.841 + 0.289840d*E [05365]. Outside outbursts Z Cam |the light curve is modulated with spectroscopic elements Z Cam |and has a shoulder at the phase 0.88P and a broad, shallow Z Cam |dip at the phase 0.15P. Outside maxima flickering up to Z Cam |0.5m with P ~ 16s - 18s is observed. During maxima Z Cam |brightness fluctuations are small [05365,04193]. RS Cam |Mean brightness varies. RU Cam |[A/H] = +0.9:. P var. Min = 2417610.1 + 22.187d*E (1908 - RU Cam |1917), Min = 2421315.3 + 22.121d*E (1917 - 1922), RU Cam |Min = 2423195.6 + 22.217d*E (1922 - 1931), Min = RU Cam |2426350.4 + 22.138d*E (1931 - 1951), Min = RU Cam |2433700.2 + 22.162d*E (1951 - 1961), Min = RU Cam |2437356.9 + 22.055d*E (1961 - 1965) [03243]. RU Cam |Unusual variable. The shape of the light curve varies. RU Cam |Before 1964 broad maxima and sharp minima were observed; RU Cam |Delta(m) varied by the factor of 2, with a possible cycle RU Cam |5.1a [03241]. After 1964 - 1966 Delta(m) decreased abruptly RU Cam |(to 0.4m - 0.1m and smaller), the light curve became RU Cam |symmetric; the mean light varies in the range of 0.3m B. RU Cam |The period varies irregularly in the interval RU Cam |19.4d - 23.5d. Groups of oscillations are observed to RU Cam |replace one another, with phase shifts up to 0.5p [04206]. RU Cam |Unusual spectrum with intense CN and weak C2 bands. RW Cam |[A/H] = +0.4. P var? RX Cam |B - V: +1.05, +1.48. [A/H] = 0. RY Cam |Possibly P2 = 150.8d. SS Cam |d = 0.06P. Min II 10.35:. P var; nonlinear term: SS Cam |+2.04d*10**(-9)*E**2. SV Cam |Depth of Min II 0.15m: pg. P var. A cycle of 50a may be SV Cam |present in period changes. The elements in the Table are SV Cam |valid since 1967.5. SW Cam |P var. Before JD2437600 Max = 2434448 + 254.2d*E. Since SW Cam |JD2440000 - see Table. SZ Cam |Member of the open cluster NGC 1502. ADS 2984 B (A = NSV SZ Cam |1458 7.1m V; B 18", 304deg). Min II 7.24, D II = 0.17P. SZ Cam |P var. Since 1970 - see Table; earlier SZ Cam |Min I = 2427533.5191 + 2.6984166d*E [02071]. TU Cam |Min II 5.22. TV Cam |[A/H] = -0.2. TX Cam |SiO maser. UY Cam |Delta(m) var (0.2m - 0.5m V) [03528]. UZ Cam |P var? Before JD2428700 Max = 2427992 + 231.0d*E [00114]; UZ Cam |since JD2440000 - see Table. WW Cam |d = 0.013d. Min II 11.1. XX Cam |During 1898 - 1980 a single symmetric Min JD2429632 was XX Cam |observed which lasted for 94d. Brightness fluctuations up XX Cam |to 0.2m during several dozens of minutes [04271]. Hydrogen XX Cam |deficiency and carbon excess in the spectrum. Some authors XX Cam |express doubt about the star's being an RCB variable; in XX Cam |particular, they note the lack of IR excess [05423,05430]. AB Cam |[A/H] = -0.1. AD Cam |[A/H] = -1.0. AE Cam |Min II 15.8. AH Cam |VB A (B 7"). P var. Max = 2433897.519 + AH Cam |0.3687404d*E (JD2427000 - 33897) [02305]. Since AH Cam |JD2438000 - see Table. Magnitude in Max varies with a AH Cam |possible cycle Pi = 46 P [03506]. AK Cam |P var. Min = 2426393.180 + 2.226780d*E (JD2426390 - 36610) AK Cam |[02594]; since JD2436000 - see Table. AS Cam |d = 0.009P. Min II 8.97, DII = 0.06P, Min II - Min I = AS Cam |0.437P. AT Cam |Min II 10.6. AU Cam |Very red. AV Cam |d = 0.04P. AW Cam |Min II 8.36. AX Cam |Detailed spectral studies [07191], [07192]. AY Cam |Min II 10.23, DII = 0.12P, dII = 0.02P. According to AY Cam |[03260], the spectrum is A5. AZ Cam |Min II 10.8. BI Cam |Delta(m) = 0.9m pg. BK Cam |During 1912 - 1932 periodic (P ~4.4a) spectral changes BK Cam |were observed which came to an end by 1937 [04282]. BM Cam |SB1 (P = 80.174469d; e = 0.35). Epoch of Min light is given. CZ Cam |P = 267.79d, semiregular behavior unusual for B5 stars. R Cnc |SiO maser. S Cnc |In the field of Praesere (NGC 2632) cluster. d = 0.015P. S Cnc |Min II 8.39. P var. U Cnc |VB A (B 3"). In the field of Praesepe (NGC 2632) cluster. V Cnc |S0.5/6e. ADS 6763 A (B 13.5m, 10", 270deg). RS Cnc |P2 = 1700d. Tc lines are present in the spectrum. RT Cnc |P2 ~600d. RU Cnc |d = 0.035P. Min II 10.21:, DII <= 0.07P. RW Cnc |P var. Since JD2437000 - see Table. According to [02088], RW Cnc |Max = 2421339.380 + 0.5471932d*E + RW Cnc |0.57d*10**(-9)*(E - 5800)**2 + 0.028d*cos0.0215deg* RW Cnc |(E + 2260) + f(psi, hi); here the last term is the sum of RW Cnc |two short period oscillations and is given in graphical RW Cnc |form, since the main period (0.547d) varies with RW Cnc |Pi1 = 29.9d and Pi2 = 91.1d. Magnitude in Max varies from RW Cnc |10.7m to 11.8m, in Min from 12.3m to 12.6m. RY Cnc |In the region of the open cluster NGC 2632 (Praesepe), RY Cnc |non-member. B - V: +0.58, +1.05. P var. Before JD2436000 RY Cnc |Min = 2429334.445 + 1.0929500d*E; since RY Cnc |JD2436000 - see Table. RZ Cnc |Min II 9.21. d = 0.015P:. Ellipsoidal components. SS Cnc |Delta(S) = 1.2. P var? SV Cnc |B - V: +0.10, +0.52. SY Cnc |Flickering with P ~20s - 34s [05959]. Spectral investigation SY Cnc |[04286]. TT Cnc |(k - b)2 = 0.11. P var. Before JD2430700 TT Cnc |Max = JD2425647.452 + 0.5634445d*E [03506]. TT Cnc |Since JD2439800 - see Table. Blazhko effect, Pi = 89d TT Cnc |[05271]. TW Cnc |d = 0.014P. Depth of Min II 0.1m pg. TX Cnc |Member of the open cluster Praesepe (NGC 2632). Min II TX Cnc |10.32. TY Cnc |d = 0.013P. P var. UU Cnc |Min II 9.2, JD (Min II) 2435608.5. SB1. The light curve is UU Cnc |unstable. Spectral studies [01881], [03149], [04289]. UV Cnc |In the region of the Praesepe (NGC 2632) cluster. UZ Cnc |Min II 11.4. VY Cnc |Min II 12.3:. VZ Cnc |(k - b)2 = 0.32. Beat phenomenon for two oscillations is VZ Cnc |observed. According to [02125], for the middle of VZ Cnc |the ascending branch T (<m>) = 2433631.84615 + VZ Cnc |0.17836376d*E + 0.00193d*sin(2*pi*psi(<m>) - VZ Cnc |0.00371d*cos*2*pi*psi(<m>); here the phase of the beat VZ Cnc |period psi(<m>) is computed with the elements T(<m>) = VZ Cnc |Spectral investigation [02126]. WW Cnc |According to [07531], the period does not vary since 1933. WW Cnc |A number of minima by WW Cnc |BBSAG contradict the tabulated elements. WX Cnc |Min II 10.7. WY Cnc |VB A (B 12.8m, -20", 0deg). Min II 9.60. XX Cnc |In the region of the Praesepe (NGC 2632) cluster. XZ Cnc |Min II 10.2. YY Cnc |According to [03263], the star is probably an irregular YY Cnc |variable. YZ Cnc |Oscillations with P = 133.2m are observed in maximum light YZ Cnc |[06249]. ZZ Cnc |d = 0.02P:. AC Cnc |Min II 14.7. <Max> = 14.5. AC Cnc |The brightness outsibe eclipses varies in the range 13.8 - AC Cnc |15.2B. 3 deep minima contradict the tabulated AC Cnc |elements [04460]. The identification with the X-ray AC Cnc |source H 0857+13 is not excluded. AD Cnc |Min II 13.4. AH Cnc |Member of the open cluster M 67 (NGC 2682). Min II 13.68. AH Cnc |Nonlinear term: +1.56d*10**(-10)*E**2. AH Cnc |Cyclic period variations (with different cycles) are also AH Cnc |possible [04475]. AO Cnc |Min II 13.4. AP Cnc |P var? AU Cnc |Possible member of the cluster praesepe (NGC 2632). AV Cnc |Possible member of the cluster Praesepe (NGC 2632). AW Cnc |Possible member of the cluster Praesepe (NGC 2632). AX Cnc |Possible member of the cluster Praesepe (NGC 2632). AY Cnc |Possible member of the cluster Praesepe (NGC 2632). AZ Cnc |Possible member of the cluster Praesepe (NGC 2632). BB Cnc |Delta(mu) > 6.0. Possible member of the cluster BB Cnc |Praesepe (NGC 2632). BC Cnc |Delta(mu) > 4.0. Possible member of the cluster BC Cnc |Praesepe (NGC 2632). BD Cnc |Possible member of the cluster Praesepe (NGC 2632). BE Cnc |Possible member of the cluster Praesepe (NGC 2632). BG Cnc |Possible member of the cluster Praesepe (NGC 2632). BH Cnc |Possible member of the cluster Praesepe (NGC 2632). BI Cnc |The elements were determined by Winzer. Epoch of Max BI Cnc |in U band is given. BK Cnc |Possible member of the cluster Praesepe (NGC 2632). BM Cnc |SB (P = 585.4154d [06568]). The elements in the Table BM Cnc |represent the moments of maximal (B - V). BN Cnc |Member of the cluster Praesepe (NGC 2632). BQ Cnc |SB.Member of the cluster Praesepe (NGC 2632). BR Cnc |VB A (B 14.2m, 30", 268deg). Member of the cluster BR Cnc |Praesepe (NGC 2632). BS Cnc |Member of the cluster Praesepe (NGC 2632). BT Cnc |Member of the cluster Praesepe (NGC 2632). BT Cnc |Oscillations with other periods are superimposed. BU Cnc |Member of the cluster Praesepe (NGC 2632). According to BU Cnc |[04483], P = 0.071d is not confirmed; during different BU Cnc |nights P = 0.0534d, P = 0.059d and several other BU Cnc |periodicities were observed. BV Cnc |Member of the cluster Praesepe (NGC 2632). BW Cnc |Member of the cluster Praesepe (NGC 2632). BX Cnc |Member of the cluster Praesepe (NGC 2632). BY Cnc |Member of the cluster Praesepe (NGC 2632). BZ Cnc |In the region of the Praesepe (NGC 2632) cluster. CC Cnc |Cycle <= 90d. CD Cnc |Possible member of the cluster Praesepe (NGC 2632). CE Cnc |In the region of the Praesepe (NGC 2632) cluster. CF Cnc |In the region of the Praesepe (NGC 2632) cluster. CG Cnc |In the region of the Praesepe (NGC 2632) cluster. CH Cnc |In the region of the Praesepe (NGC 2632) cluster. CI Cnc |Possible member of the cluster Praesepe (NGC 2632). CK Cnc |In the region of the Praesepe (NGC 2632) cluster. CL Cnc |In the region of the Praesepe (NGC 2632) cluster. CM Cnc |Possible member of the cluster Praesepe (NGC 2632). CN Cnc |Possible member of the cluster Praesepe (NGC 2632). CO Cnc |In the region of the Praesepe (NGC 2632) cluster. CP Cnc |In the region of the Praesepe (NGC 2632) cluster. CR Cnc |In the region of the Praesepe (NGC 2632) cluster. CS Cnc |In the region of the Praesepe (NGC 2632) cluster. CU Cnc |G 9-8 = G 40-25. VB A (B = CV Cnc, 13", 347deg), CU Cnc |common mu. In the region of Praesepe (NGC 2632) cluster, CU Cnc |non-member. CV Cnc |G 40-26. VB B (A = CU Cnc). CY Cnc |Member of the cluster Praesepe (NGC 2632). CZ Cnc |Equinox in [08354] must be 2000.0. DD Cnc |In the region of the Praesepe (NGC 2632) cluster. DF Cnc |In the region of the Praesepe (NGC 2632) cluster. DF Cnc |Posibly non-member. DG Cnc |In the region of the Praesepe (NGC 2632) cluster. DG Cnc |Possibly non-member. DH Cnc |Possible member of the cluster Praesepe (NGC 2632). DI Cnc |Possible member of the cluster Praesepe (NGC 2632). DL Cnc |VB. In the region of the Praesepe (NGC 2632) cluster. DM Cnc |Possible member of the cluster Praesepe (NGC 2632). DN Cnc |In the region of the Praesepe (NGC 2632) cluster. DO Cnc |In the region of the Praesepe (NGC 2632) cluster. DP Cnc |In the region of the Praesepe (NGC 2632) cluster. DQ Cnc |In the region of the Praesepe (NGC 2632) cluster. DQ Cnc |Possibly non-member. DR Cnc |In the region of the Praesepe (NGC 2632) cluster. DS Cnc |In the regiom of the Praesepe (NGC 2632) cluster. DS Cnc |Possibly non-member. DT Cnc |In the region of the Praesepe (NGC 2632) cluster. DU Cnc |In the region of the Praesepe (NGC 2632) cluster. FV Cnc |The type is doubtful. kap Cnc |SB (P = 6.39316d). In [04487] the light variability was not kap Cnc |confirmed. R CVn |P var. Max = 2411768 + 325.4d*E (JD2411730 - 26430) [01701]; R CVn |Max = 2432074 + 332.8d*E R CVn |(JD2426750 - 32100); since JD2432100 - see Table. T CVn |SRA? Delta(m) strongly varies. U CVn |OH, H2O emission. V CVn |H2O, SiO maser. W CVn |B - V: +0.15, +0.42. P var. W CVn |Nonlinear term: -368*10**(-13)*E**2. Delta(S) = 7. Y CVn |P2 = 2000d. Z CVn |B - V: +0.20, +0.33. P var. Max = 2413000.262 + Z CVn |0.6538236d*E (JD2413000 - 23170); Max = Z CVn |2423860.355 + 0.6539052d*E (JD2423860 - Z CVn |31800) [01702]; Max = 2432943.645 + 0.653824d*E Z CVn |(JD2431800 - 40200) [06457]. Since JD2438900 - see Table. Z CVn |Blazhko effect: Min. ampl. = 2439176.12 + 22.75d*E [03267]. Z CVn |Amplitude varies by 0.5m B, extremal periodic deviations Z CVn |of the epoch of Max from linear elements are +-0.02d. Z CVn |Delta(S) = 8. RR CVn |B - V: +0.09, +0.45. [Fe/H] = -1.33. RR CVn |The light curve shape and Delta(m) var. RS CVn |Min II 8.19; Min II - Min I = 0.506P; d = 0.033P. RS CVn |P var. Nonlinear term: -1.00d*10**(-8)*E**2. Wave-like RS CVn |distorsion with the amplitude from 0.09m up to 0.20m and RS CVn |with the period 4.7917d close to the orbital one is RS CVn |observed on the light curve out of eclipses [07209]. RS CVn |The wave is migrating on phase in the direction of phase RS CVn |decreasing with a migration period of 9.48 years [05800]. RU CVn |B - V: +0.10, +0.39. P var. Max = 2420227.338 + RU CVn |0.5732502d*E (JD2418801 - 29436) [05436]; Max = RU CVn |2420227.398 + 0.57324647d*E (JD2418979 - RU CVn |36665) [03271]; since JD2434483 - see Table. RV CVn |V141 (M3/NGC 5272). Not a member of the cluster. RV CVn |Min II 15.81. RX CVn |B - V: +0.17, +0.41. P var? RZ CVn |B - V: +0.12, +0.43. P var. Max = 2424621.489 + RZ CVn |0.56740036d*E (JD2424620 - 31000) [00188]; RZ CVn |Max = 2437823.433 + 0.5674174d*E (JD2434470 - RZ CVn |37830); since JD2438200 - see Table. ST CVn |P var? Delta(S) = 4.8. SV CVn |P var. Max = 2427434.911 + 0.66805653d*E SV CVn |(JD2426000 - 32000) [00752]; since JD2439500 - see Table. SW CVn |P var. Max = 2431139.791 + 0.44164922d*E SW CVn |(JD2425640 - 32000) [00752]; since JD2436200 - see Table. TX CVn |SB2 (P = 70.8d) [04504]. UU CVn |In the region of the globular cluster NGC 5466. P var. UU CVn |Max = 2437817.312 + 0.5409589d*E (JD2436360 - 39945); UU CVn |since JD2439945 - see Table. UV CVn |In the region of globular cluster NGC 5466, non-member. UV CVn |P var. Max = 2419446.156 + 0.6316090d*E (JD2419440 - 34455); UV CVn |since JD2434450 - see Table. UW CVn |In the region of the globular cluster NGC 5466. UX CVn |Min II 11.94. U - B: -1.05, -0.99; B - V: -0.29, -0.23. VV CVn |Min II 14.3:. VW CVn |Min II 12.4. P var. Min I = 2435923.246 + 0.8499757d*E VW CVn |(JD2427900 - 36000); since JD2435900 - see Table. The VW CVn |variable is not marked on the map. It is by 6mm to the VW CVn |west and 3mm to the north of the comparison star C. VZ CVn |Min II 9.54. WW CVn |Blazhko effect is possible. WY CVn |V 205 (M3/NGC 5272). Member of the cluster? Blazhko effect WY CVn |is possible. WZ CVn |V 206 (M3/NGC 5272). Non-member? Blazhko effect. XX CVn |In the region of M3 (NGC 5272) globular cluster. Member XX CVn |of the cluster? YZ CVn |d = 0.055P, depth of Min II 0.05m vis. AA CVn |[Fe/H] = -1.78. AD CVn |[Fe/H] = -1.39. AF CVn |[Fe/H] = -1.19. AG CVn |[Fe/H] = -2.01. AH CVn |[Fe/H] = -2.01. AI CVn |Radial multiperiod pulsations: P0 = 0.2085d, AI CVn |P1 = 0.1529d, P2 = 0.1259d, P3 = 0.1158d. AK CVn |[Fe/H] = -1.19. AM CVn |The light curve is a double wave. Min II sometimes AM CVn |disappears. The depth of Min I changes also. Epoch of AM CVn |Min I is given in the Table. P var; dP/dt = +0.012s per AM CVn |year. Elements for 1978 are given in the Table. The AM CVn |brightness fluctuates with the cycle of 115 - 120s, AM CVn |sometimes the periodicity with P = 26.3s is observed. AM CVn |Probably it is a close binary semidetached system of two AM CVn |white dwarfs with an accretion disk and a hot spot. AN CVn |[Fe/H] = -1.54. AQ CVn |Similar to horizontal branch stars in globular clusters. AQ CVn |A flare lasting 20 minutes was observed. BF CVn |G 123-75 = G 164-32. VB A (B = G 164-31, 13.16m, BF CVn |dM3.5e; 17", 225deg). Flares in the combined light of the BF CVn |system (Delta(U) up to 0.95m) were observed. BG CVn |P1 = 1186s, P2 = 780s. BH CVn |SB. Reflection effect Delta(m) = 0.013V. BI CVn |Min II 10.70. P var? CS CVn |HIPPARCOS data contradict the luminosity class V. alf 2 CVn |VB A (B 5.60m, F0V, 19.6", 228deg). alf 2 CVn |Epoch of Min is given. R CMa |Min II 5.78. P var [03280,06314]. R CMa |The star shows anomalies of the light curve [03281,03282]. V CMa |VB B (A = CPD -31deg 1311, 9.4 m; B 16", 90deg). Z CMa |Strong IR excess. Shell spectrum. Several lines show P Cyg Z CMa |profiles. The star is located in a nebula rich in details. Z CMa |A bright wisp of nebulosity near the star has continuons Z CMa |spectrum, probably identical to that of the star [04002]. RR CMa |Min II 13.1. RT CMa |Min II 11.5. RT CMa |P = 1.293745d is possible taking into account the epoch RT CMa |from [03283]. RX CMa |d = 0.027P. Min II 11.1. P var. During JD2441700 - 43000 RX CMa |- see Table. RZ CMa |P var? Since JD2435500 - see Table. SW CMa |Min II 9.9. Min II = JD2426709.366; Min II - Min I = SW CMa |0.316P. SX CMa |Min II 10.3. TU CMa |Min II 10.1. UW CMa |Min II 5.25. Gaseous streams, expanding gaseous envelope. UW CMa |Minima are asymmetric; other peculiarities of the light UW CMa |are observed. A number of spectral lines have P Cyg UW CMa |profiles. UW CMa |The line profiles are observed to vary with the phase of UW CMa |the orbital period, and also ([07227], according to Sanyal) UW CMa |with characteristic time <1h. UX CMa |Min II 12.3. VW CMa |Min II 9.1. VY CMa |ADS 6033 A (B 9.2m, 0.5", 168deg; C 11.5m, 2.7", 291deg, VY CMa |D 11m, 2.9", 347deg, ...). H2O, OH, SiO maser. VY CMa |B - V: +2.3. VY CMa |In the region of the VY CMa |young open cluster NGC 2362. Embedded in a VY CMa |reflecting nebula. The companions may be details VY CMa |of the nebula; some of them are probably variable [02159, VY CMa |03287]. Surrounded by an envelope of gas and dust or a disk VY CMa |of 0.45" (lambda = 5 mkm) angular size. Secular decrease VY CMa |of brightness since 1801. Cyclic variations of brightness VY CMa |with Delta(m) from several tenths of a magnitude to 3m on VY CMa |time scale from 200d to 1900d. TiO and ScO emission bands VY CMa |in the spectrum. Spectroscopic studies [03287,05282,06133]. WW CMa |RR, Max = 2428570.09 + 0.499355d*E [00613]. CEP, WW CMa |Max = 2428146.6 + 5.7660d*E [00514]. These systems of WW CMa |elements are contradicted by 94 photographic observations WW CMa |(Erleksova) and 12 photoelectric observations (Irwin, WW CMa |[03288]). XY CMa |d = 0.04P:. ZZ CMa |Min II 13.0. AE CMa |d = 0.02P:. AN CMa |d = 0.02P:. AO CMa |In the field of the open cluster Ruprecht 18. AR CMa |d = 0.025P:. AS CMa |d = 0.04P. BN CMa |Min II 14.9. BQ CMa |In the region of the open cluster NGC 2354. BS CMa |Min II 14.5. CC CMa |Mean brightness varies? CE CMa |Min II 13.3. Min II - Min I = 0.663P. CH CMa |Min II 12.9. CK CMa |Min II 15.4. CM CMa |Min II 13.1. CO CMa |Mean brightness probably varies with P ~700d. CR CMa |Min II 12.4. CV CMa |Min II 13.5. DII = 0.09P. Min II - Min I = 0.358P. CW CMa |Min II 8.94. SB2. CX CMa |Min II 10.3. DD CMa |Min II 11.8. DE CMa |Min II 13.4. DS CMa |VB A (B 15.8m, 10", 130deg). DV CMa |JD2425300 - 27500: P - see Table; since JD2428000 P ~400d. EF CMa |d = 0.02P. EW CMa |VB Delta(m) <= 0.5m, 0.102", 112.1deg, 1952.203). EW CMa |SB (P = 0.261975d). Brightness variations are not related EW CMa |to the orbital phase. Shell star (probably an extended EW CMa |atmosphere of one of the components and the common shell EW CMa |around the system). Spectral studies {4592 - 4596}. EX CMa |Was faint for 2 nights (October 8 and 9, 1962). EY CMa |P var, Delta(m) var [03960]. The main wave is superimposed EY CMa |by secondary ones (P = 0.2033d and 0.1690d); beat effect, EY CMa |Pb ~2.00d [07243]. EZ CMa |SB. In the centre of the ring HII region S 308. Member of EZ CMa |the open cluster collinder 121. Epoch of Max light is EZ CMa |given. The companion is probably a neutron star. The shape EZ CMa |of the light curve, Delta(m), phases of maxima and minima EZ CMa |and mean light vary from one observational season to EZ CMa |another. FF CMa |Min II 7.6. Elements should be improved. Member of the FF CMa |open cluster Cr 132a. FM CMa |Min II is almost as deep as Min I [06585]. FN CMa |VB (6.3m, 7.5m, 0.561", 115.8deg, 1978.15). Range of FN CMa |combined light variation is given in the Table. FN CMa |Associated with the nebula vB 95. According to [06135], FN CMa |the period considerably differs from the tabulated value. FQ CMa |Min II 9.7. FR CMa |ADS 4978 AB (6.2m, 10.4m, 4", 23deg; C 11.62m, 56"). FS CMa |Extended shell of gas and dust. Emissions of [FeII], FS CMa |[NiII], [CrII], [SII], [OI], FeII. IR excess FS CMa |(1.6 - 20 mkm). P Cyg profiles of Balmer lines vary in the FS CMa |time scale of hours. Brightness varies from night to night FS CMa |by 0.1m and during a night by 0.03m, sometimes in FS CMa |correlation with spectral changes [06636]. Spectral FS CMa |studies [07250,07251,07253]. FT CMa |VB A (B 12.58m, 36", 97deg). FU CMa |VB A (B 14.7m, 14", 230deg, 1897; C 11.07m, 40", 225deg). FW CMa |VR var, P = 31.9045d [06154]. FZ CMa |Min II 8.44. In the HII region S 295, in the association FZ CMa |CMa OB1. GG CMa |Member of the open cluster Cr 132a. GU CMa |ADS 5713 AB (7.5m, 8.2m, 0.6", 187deg, 1919). SB? GU CMa |In the HII region S 293. GY CMa |According to [08380], does not vary. GZ CMa |SB2. HK CMa |Epoch of Min is given. HL CMa |1E 0643.0-1648. SB (P ~0.217d); Lx/Lopt var (0.002 - 1). IU CMa |Type LBV: is also possible. MO CMa |The amplitude can have been overestimated (M. Grenon, private MO CMa |communication). NO CMa |Type LBV: is also possible. bet CMa |In 1971 - 72 the observations were described by the bet CMa |combination of the tabulated elements (period P1) and the bet CMa |following systems of elements: bet CMa |Max = 2441296.0705 + 0.251300d*E, (P2); bet CMa |Max = 2441296.032 + 0.23904d*E, (P3); bet CMa |Max = 2441296.065 + 0.12501d*E, (P1/2); bet CMa |Max = 2441296.124 + 0.12565d*E, (P2/2). bet CMa |Beat periods: 49.198d, 5.442d, 4.900d. bet CMa |Since 1908 P1 increases, P2 decreases. 12 overtone and bet CMa |resonance periods were found in [03454]. ksi 1 CMa |ADS 5176 A (B 14.5m, 25", 147deg; C 14.0m, 29", 303deg, ksi 1 CMa |1897). sig CMa |ADS 5719 A (14.2m, 11", 153deg, 1926). tau CMa |SB, Porb = 154.90d. ome CMa |SB? R CMi |SC4/10e. T CMi |P var. Max = 2422456 + 324.2d*E (JD2416610 - T CMi |22800); Max = 2430896 + 311.2d*E (JD2423090 - T CMi |30900); since JD2430900 - see Table. U CMi |There is a hump on the ascending branch looking sometimes U CMi |as a secondary maximum. The light curve for 1904 - 1970 U CMi |[07368]. X CMi |P var? Delta(S) = 3. RS CMi |d = 0.02P:. RX CMi |Min II 14.6; Min II - Min I = 0.52P:. RY CMi |Min II 12.0:. SX CMi |DI <= 0.12P. Min II 13.6. SY CMi |P var. Max = 2425234.682 + 0.565900d*E (JD2425234 - 708); SY CMi |since JD2436586 - see Table. TU CMi |Min II 15.1. TW CMi |Min II 15.6. TX CMi |Min II 14.7. UZ CMi |Min II 12.1. XZ CMi |Min II 9.88. P var? YY CMi |Min II 8.88. YZ CMi |mu = 0.604", P = 221.4deg. Epoch of Min is given. P var; YZ CMi |additional term: -0.00003919514d*E*(E + 1)/2. Periodical YZ CMi |light variations with the amplitude 0.12m (11.26 - 11.38 V) YZ CMi |are superimposed by strong flares. AG CMi |P var. Min = 2434698.670 + 1.6645729d*E (JD2426350 - AG CMi |34740) [01727]. Since JD2437650 - see Table. AH CMi |EW? AK CMi |Min II 10.3; Min II - Min I = 0.55P. P var. Min I = AK CMi |2425352.348 + 0.56589534d*E (JD2424880 - AK CMi |35550) [01728]. Since JD2435600 - see Table. AL CMi |Observations in the interval JD2424880 - 25950 are AL CMi |represented by the elements: Max = 2425243.631 + 0.55050d*E. AL CMi |Since JD2436590 - see Table. AM CMi |Min II 10.5. AN CMi |d = 0.02P:. AO CMi |d = 0.01P:. Min II 14.5. BF CMi |Depth of Min II 0.05m:. BO CMi |Several episodes of outburst-like activity. RS Cap |Mean brightness varies with P = 3360d. RT Cap |VB A (B 15m, 26", 227deg). RU Cap |VB A (B 13.6m, 1.6", 86deg). RV Cap |<P> var: Max = 2424334.6612 + 0.44775262d*E RV Cap |(JD2417400 - 33610) [00323]. Since JD2433850 - see Table. RV Cap |Light curve and period vary with the Blazhko effect RV Cap |period Pi = 225.5d [06464]. Semiamplitude of deviations RV Cap |from linear elements is +-0.032d. 0.14P <= M - m <= 0.25P. RV Cap |(k - b)2 = 0.05. RW Cap |d = 0.020P. Min II 9.9. P var. Min I = 2418924.594 + RW Cap |3.3923922d*E (JD2418920 - 24000) [06774]; RW Cap |Min I = 2424003.014 + 3.3923457d*E (JD2424000 - RW Cap |34500) [02389]; since JD2435400 - see Table. RX Cap |Min II 12.5. RY Cap |VB B (A 7.1m, F0; B 6.6", 90deg; C 12.0m, 8.5", 58deg). TV Cap |<P> = 67d [01331]. TW Cap |P var. P = 28.6421871d (JD2414000 - 17600); TW Cap |P = 28.61700115d (JD2417600 - 24000) [01331]; TW Cap |Max = 2426211.90 + 28.59497d*E (JD2421400 - TW Cap |26200) [02390]; Max = 2435664.8 + 28.5578d*E TW Cap |(JD2426210 - 37500) [02309]; since JD2437500 - see Table. TW Cap |0.14P <= M - m <= 0.40P. [Fe/H] = -0.72. TY Cap |Min II 10.6. P var. Min I hel = 2432017.956 + 1.423466D*E TY Cap |(JD2425500 - 35000); since JD2435000 - see Table. UW Cap |Min II 11.5; Min II - Min I = 0.5P. P var? Min I = UW Cap |2434627.290 + 1.399118d*E (JD2427000 - 35000); UW Cap |since JD243500 - see Table. YZ Cap |(k - b)2 = 0.08. AD Cap |Outside eclipses B - V = +1.00. P var? AE Cap |Mean brightness varies with P = 2300d. BH Cap |Type RR: is also possible. BN Cap |The variability may be due to the fainter (B) component. del Cap |VB A (B 15.8m, 69", 94deg; C 12.7m, 119", 302deg, del Cap |1911); mu = 0.391", P = 138.8deg. Min II 2.90. del Cap |The light curve shape var? [03305]. eps Cap |VB A (B 9.52m, 68.7", 47deg). R Car |VB A (B 12m, 2.1", 138deg). H2O, SiO maser. U Car |P var. Max = 2429023.80 + 38.753d*E (JD2415000 - U Car |29500); since JD2429500 - see Table. V Car |The light curve shape var? X Car |Min II 8.6. Y Car |VB A (B 12.22m, 15"; C 12.96m, 30"). SB (P = 400 - 600d) Y Car |[05119]. The fundamental mode period P0 is given in the Y Car |Table (A = 0.58m). The first overtone period P1 = 2.55954d Y Car |[05119] (A = 0.28m). P1/P0 = 0.7032. RR Car |P var. <P> = 154d (JD2421500 - 23500); <P> = 259d RR Car |(JD2426400 - 30100); <P> = 154d (JD2430400 - 33100). RR Car |S6.5/1- . RT Car |In the region of the cluster Tr 15. RY Car |There is a close companion 14.3 pg. P var. RY Car |Max = 2418475 + 416d*E (JD2415140 - 18500); RY Car |Max = 2429901 + 417.3d*E (JD2423600 - 32900); RY Car |since JD2434100 - see Table. ST Car |Depth of Min II 0.27m. SW Car |Depth of Min II 0.05m. SZ Car |In the region of the cluster NGC 3114. TX Car |The light curve shape var? TZ Car |Mean brightness varies with P = 1183d; the amplitude of TZ Car |the short cycle is large in mean brightness maximum and TZ Car |small during its minimum. UX Car |In the region of the cluster IC 2581. VV Car |In the region of the very poor cluster N 99 [07374] VV Car |(10h 36.0m -58deg 56', 1950.0) embedded in a nebula. VY Car |VB A (B 11.07m; B 9V:, 10", 150deg). P var. VY Car |Nonlinear term: -0.000021d*E**2 (JD2410000 - 44200). VY Car |The latest observations may be represented also by linear VY Car |elements: Max = 2444161.16 + 18.9138d*E VY Car |(JD2441000 - 44200). [A/H] = 0.4. WZ Car |P var. Max = 2419981.099 + 23.000945d*E (JD2410000 - 20000) WZ Car |[00025]; Max = 2423984.12 + 23.0054d*E (JD2419800 - 25500) WZ Car |[00322]; Max = 2434914.86 + 23.0075d*E + 0.000025d*E**2 WZ Car |(JD2434500 - 41200) [02309]; since JD2434500 - see also WZ Car |Table. XX Car |P var. Max = 2420769.703 + 15.723704d*E (JD2410000 - 22500) XX Car |[00025]; P = 15.7196d (JD2423000 - 30000) [00003]; since XX Car |JD2434500 - see Table; elements given in the Table contain XX Car |a nonlinear term: -0.0000034d*E**2. XY Car |[A/H] = 0.1. XZ Car |[A/H] = 0.2. YZ Car |P var. Nonlinear term: +0.0000022d*E**2. [A/H] = -0.1. AE Car |In the region of the cluster NGC 3532. AF Car |P var. Max = 2434532 + 433.7d*E (JD2420200 - 34600); since AF Car |JD2435000 - see Table. AG Car |Central star of the low-excitation planetary nebula AG Car |P.K.289-0.1 ejected probably during a nova-like outburst AG Car |of the star about 1000 years ago [07052,07113]. AS Car |d = 0.025P. AW Car |d = 0.015P. BL Car |In the region of the cluster Tr 16. BO Car |VB A (B 11.05m V, B8III, 10", 41deg). In the region of BO Car |the cluster Tr 15. Cluster non-member. BP Car |P = 4.82246d? BS Car |In the region of the cluster IC 2602. Min II 15.3. BZ Car |Mean brightness possibly varies with P = 1800d. CD Car |In the centre of the cluster Cr 236. CF Car |In the region of the cluster NGC 3496. CI Car |In the region of the cluster NGC 3572. d = 0.021P? CO Car |d = 0.024P? CV Car |d = 0.046P. Depth of Min II 0.05m. DE Car |d = 0.016P? DH Car |VB B (A 15.2m V; B 13", 350deg). B - V = +0.90m DH Car |(Min brightness). DI Car |Besides Cepheid-like light variations with the amplitude DI Car |1.7m and elements Max = 2438553.70 + 29.210d*E DI Car |(JD2438465 - 40300) [05324] large weakenings of brightness DI Car |are observed [04678]. At Max B - V = +1.34. DK Car |d = 0.07P. DM Car |d = 0.040P. DP Car |d = 0.034P. Min II 13.1. DS Car |d = 0.03P. DU Car |In the region of the cluster IC 2602. DW Car |In the region of the cluster Cr 228. Min II 10.3. EF Car |d = 0.04P. EG Car |In the region of the cluster NGC 3532. EH Car |VB A (B 15", 320deg). EK Car |In the region of the cluster NGC 3532. EM Car |Min II 8.9. EN Car |In the region of the cluster Tr 18. EQ Car |d = 0.030P. Min II 13.7. ER Car |In the region of the cluster NGC 3532. ES Car |In the region of the cluster NGC 3572. EZ Car |Min II 9.8. FI Car |P var. Max = 2425446.81 + 13.4542d*E (JD2423790 - 35300) FI Car |[00046,02309]. Since JD2435300 - see Table. FK Car |VB. FO Car |VB A (B 14m, 7", 90deg). P var. Max = 2434922.531 + FO Car |10.3559d*E (JD2423700 - 35300) [06006]; since JD2436000 FO Car |- see Table. B - V: +1.13, +1.43. FP Car |d = 0.01P:. FQ Car |In the region of the cluster Tr 18. FS Car |In the region of the very poor cluster N 99 [07374] (10h FS Car |36.0m -58deg 56', 1950.0) embedded in a nebula. Min II FS Car |10.9. FT Car |According to [02197] spectrum C. Misidentification is FT Car |possible. FV Car |VB A (B 13m, 10", 135deg). P var. There are two additional FV Car |terms in the elements given in the Table: FV Car |-0.1065d*10**(-7)*E**2 - 0.584d*10**(-11)*E**3. FV Car |d = 0.02P:. Min II 13.0. GG Car |Min II 9.5. Gas and dust envelope. GH Car |In the region of the cluster Tr 18. GK Car |In the region of the cluster Tr 19. Min II 13.2. GL Car |In the region of the cluster NGC 3572. Min II 10.31. GL Car |System with the apsidal motion; e = 0.157, omega = 99deg. GL Car |There are sinusoidal terms in the elements for Min I given GL Car |in the Table: +0.121d sin(0.094389deg*E) - GL Car |0.007d sin(0.188778deg*E); GL Car |Min II = 2424263.236 + 2.4222338d*E - GL Car |0.121d sin(0.094389deg*E) - 0.007d sin(0.188778deg*E). GL Car |DII = 0.17P. GM Car |In the region of the very poor cluster N 99 [07374] (10h GM Car |36.0m -58deg 56', 1950.0) embedded in a nebula. GM Car |Min II 9.22. GN Car |Min II 12.1. GO Car |VB A (B 15", 60deg). GP Car |Min II 12.8. GQ Car |Min II 13.5. GR Car |Min II 14.0; Min II - Min I = 0.316P; DII = 0.05P. GV Car |Possible member of the cluster NGC 3532. Min II 9.1. GW Car |Min II 9.9. GZ Car |Light elements for the fundamental mode oscillation with GZ Car |an amplitude 0.16m are given in the Table. For the first GZ Car |overtone oscillation with an amplitude 0.07m GZ Car |Max = 2440742.4 + 2.93424d*E. Epochs of maxima and GZ Car |amplitudes are given according to [05175]. HH Car |VB A (B 13.0m, 5", 260deg; C 11.11m, 13", 337deg; D 12.65m, HH Car |15", 7deg). d = 0.02P. Min II 10.66. P var [08094]. HH Car |Min I hel = 2430860.162 + 3.2315393d*E (JD2427590 - 35260) HH Car |[05292]. Possible current elements are given in the Table. HI Car |Min II 10.8. HK Car |VB A (B 12.5m, 4"). Range of combined brightness variation HK Car |is given. HL Car |d = 0.03P:. HN Car |Min II 12.5. HP Car |VB A (B 9.1m, 0.4", 178deg). Min II 9.3. Elements should HP Car |be corrected [08083]. HQ Car |B - V: +0.63, +1.04. HR Car |Spectrum description [01914,06466]. HT Car |In the region of the cluster IC 2581. Min II 14.0. HV Car |d = 0.026P. Min II 14.2. HW Car |Epoch of Min is given. HX Car |Min II 14.5. IK Car |In the region of the cluster NGC 2602. IL Car |Min II 14.4. IN Car |It is possible that the period must be doubled. IQ Car |In the region of the cluster NGC 3532. IR Car |In the region of the cluster NGC 3532. Min II 12.6. IS Car |Min II 14.0. IU Car |(k - b)2 = 0.02. IW Car |Mean brightness varies with the period close to 1500d, the IW Car |amplitude of main oscillations - from 1.3m to 0.3m. IX Car |In the centre of a bright nebula with the diameter 2.4'. IZ Car |Declination in [00085] is wrong by 3deg. Identical to IZ Car |V336 Car, see [06316]. KQ Car |Min II 10.3. KU Car |Min II 11.6. MP Car |VB A (B 16m, 180deg). MZ Car |sf component of a close pair. OO Car |Min II 14.7. OV Car |Min II 13.5. OY Car |Eclipse elements: OY Car |Min I hel = 2443993.553241 + 0.0631209247d*E [05185]; OY Car |D = 0.050P, d = 0.044P. The hump on the light curve is OY Car |observed at the phase of 0.75P. Depth of Min I varies OY Car |between 1.48m and 2.47m. PT Car |Min II 13.0:. PX Car |Min II 10.10. QR Car |Min II 10.4. QS Car |Min II 9.3. QU Car |HDE 310376 (HA 112, 173). Flickering resembles V818 Sco. QU Car |Variations by 0.2m in 90s were observed. No periodicity QU Car |was found. Emission lines He II 4686, CIV - NIII 4630 - QU Car |4650 and sometimes weak hydrogen absoptions (corresponding QU Car |to A or B type) are noticeable in the spectrum [05643]. QX Car |Min II 7.02. QY Car |In the open cluster No.90 [07374]. QZ Car |In the eta Carina nebula, possible member of the cluster QZ Car |Collinder 228. Min II 6.43. Two SB1 systems (A and B), QZ Car |B is eclipsing (A: SB1, P = 20.73d, O9.5 I, QZ Car |Delta(m) = 0.6m). Combined brightness is given. V0341 Car |In the variable reflecting nebula IC 2220. In the region V0341 Car |of the open cluster NGC 2516. IR excess. V0343 Car |VB. SB (P = 133.92d). V0347 Car |Deep Min II. V0348 Car |In the open cluster IC 2581. Min II 8.9. V0354 Car |Very red. V0356 Car |Member of the cluster NGC 2516. V0357 Car |SB (P = 6.74483d [04627]). V0361 Car |In the region of the cluster NGC 3293. V0365 Car |In the region of the cluster NGC 3532. V0367 Car |Min II 7.54. V0373 Car |Member of the cluster NGC 2516. V0374 Car |Member of the cluster NGC 2516. V0375 Car |P = 0.264d or 0.359d. V0376 Car |VB A (B 6.83m, B 9.5V, 41", 75deg). V0378 Car |In the open cluster NGC 3293. V0379 Car |In the open cluster NGC 3293. V0380 Car |In the open cluster NGC 3293. V0381 Car |In the open cluster NGC 3293. V0382 Car |In the region of the cluster NGC 3532. V0385 Car |Depth of Min II 0.04m. Surrounded by a ring nebula RCW 58. V0491 Car |Mean magnitude 9.69. V0493 Car |SB, Porb = 3.368d. V0498 Car |Type BE: is also possible. V0534 Car |Flare-like activity. eta Car |In the emission nebula NGC 3372 in the region of the eta Car |cluster Tr 16. A very massive young star surrounded by an eta Car |expanding gas and dust shell with the diameter 2" at 2mu eta Car |and 6.5" at 12.2mu. Maximum brightness was observed in eta Car |1843. Since 1880 varies in the range 5.9 - 7.9 V. In the eta Car |interval JD2434000 - 41000 Max = 2434037 + 1110d*E. There eta Car |are emission lines of H, HeI, FeII, [FeII], etc. in the eta Car |spectrum. Description of the spectrum [05251,07279]. eta Car |Soft X-ray source of variable intensity. khi Car |Soft X-ray source. R Cas |VB A (B 14.5m, 14", 273deg). SiO, OH maser; R Cas |sometimes H2O emission. T Cas |SiO maser. ZrO bands in the infrared spectral region. U Cas |S4.5/4e. W Cas |SC5/9e. X Cas |P var: Max = 2426650 + 432.32d*E (JD2416750 - 27060); X Cas |Max = 2432870 + 413.6d*E (JD2427060 - 32870); X Cas |Max = 2437948 + 423.0d*E (JD2432870 - 39210). X Cas |Current elements are given in the Table. Y Cas |OH, H2O emission; SiO maser. Z Cas |SiO maser. RS Cas |P var. Max = 2416942.16 + 6.29552d*E (JD2412650 - 34900) RS Cas |[03317]. Since JD2434900 - see Table. RV Cas |There are signs of Se type in the spectrum [03383]. RW Cas |P var. Max = 2421354.22 + 14.8004d*E (JD2417000 - 30000). RW Cas |Since JD2430000 - see Table. [A/H] = 0.3. RX Cas |Unigue rapidly evolving eclipsing system. 9.12<=Min II<=9.49; RX Cas |Min II - Min I = 0.5070P. P var. Nonlinear term: RX Cas |+1.017d*10**(-5)*E**2. Observations may be represented RX Cas |also by three systems of elements: Min I = RX Cas |2416250.889 + 32.31481d*E (0 <= E <= 286, RX Cas |JD2416250 - 25482); Min I = 2416248.835 + 32.32145d*E RX Cas |(331 <= E <= 554, JD2426940 - 34155); RX Cas |Min I = 2416244.990 + 32.32765d*E (734 <= E <= 876, RX Cas |JD2439970 - 44570). Brightness of the system out of RX Cas |eclipses periodically varies within 8.6m - 9.0m with RX Cas |elements Max = 2416198 + 516.06d*E [05036]. Max - Min = RX Cas |233d = 0.45P [00881]. Strong emissions of H, NV, CIV, RX Cas |SIIV, FeIII. Powerful gaseous stream and accretion RX Cas |phenomena are possible. RY Cas |[A/H] = 0.0. RZ Cas |Min II 6.26. The light curve shape var; d var RZ Cas |(0.000P <= d <= 0.009P). P var, variations are irregular. RZ Cas |Mean elements based on visual and photographic RZ Cas |observations: Min I = 2416886.8806 + 1.195253065d*E RZ Cas |(JD2416800 - 26700) [08820], Min I = 2432820.7853 + RZ Cas |1.1952517d*E (JD2426700 - 34000) [00938]. From RZ Cas |photoelectric observations: Min I = 2432115.5827 + RZ Cas |1.1952472d*E (JD2429870 - 30400); Min I = RZ Cas |2432085.7011 + 1.195259d*E (JD2432000 - 32460); RZ Cas |Min I = 2434349.5130 + 1.1952525d*E (JD2432450 - 34420); RZ Cas |Min I = 2434703.3035 + 1.195238d*E (JD2434420 - 34705); RZ Cas |Min I = 2435934.4087 + 1.1952499d*E (JD2434705 - 35950); RZ Cas |Min I = 2438829.2818 + 1.195243d*E (JD2436800 - 39100); RZ Cas |Min I = 2440182.3089 + 1.195259d*E (JD2439380 - 40200); RZ Cas |Min I = 2441333.3257 + 1.195244d*E (JD2440500 - 41350); RZ Cas |Min I = 2442327.7798 + 1.1952521d*E (JD2441550 - 42350); RZ Cas |since JD2442850 - see Table. SU Cas |[A/H] = -0.1. SV Cas |P var. Max = 2421839 + 279.3d*E (JD2417600 - SV Cas |21900); Max = 2430450 + 281.7d*E (JD2422500 - SV Cas |31900); since JD2432600 - see Table. SX Cas |VB A (B 11.5m, 19", 250deg, 1966). Min II 9.32. The light SX Cas |curve shape var. DII = 0.171P:, dI = 0.036P, dII = 0.050P. SX Cas |P var. Min I = 2433963.267 + 36.56727d*E (JD2418000 - SX Cas |37000); since JD2438700 - see Table. Strong emissions SX Cas |of H, NV, CIV, SIIV, FeIII. Gaseous streams and accretion SX Cas |phenomena. SY Cas |VB? P var. Max = 2417911.547 + 4.070969d*E SY Cas |(JD2417000 - 34000); since JD2434000 - see Table. SZ Cas |P var. Max = 2421261.66 + 13.6009d*E (JD2416700 - 21260); SZ Cas |Max = 2426650.20 + 13.6072d*E (JD2421260 - 27170) [08821]; SZ Cas |Max = 2429727.240 + 13.61744d*E (JD2427170 - 33050); SZ Cas |Max = 2436810.92 + 13.62655d*E (JD2433050 - 38720); SZ Cas |since JD2438720 - see Table. [A/H] = -0.6. TU Cas |Fundamental mode period P0 is given in the Table; the TU Cas |corresponding amplitude is 0.69m. First-overtone period TU Cas |P1 = 1.51830d; the corresponding mean amplitude decreased TU Cas |from 0.4m to 0.25m during 67 years [05078]. P1/P0 = 0.71. TU Cas |M - m var (0.17P <= M - m <= 0.35P). TV Cas |d = 0.01P. Min II 7.34. The light curve shape var. TV Cas |Period of these variations - 600d [08822]. P var. Mean TV Cas |elements based on visual and photographic observations: TV Cas |Min I = 2432827.7665 + 1.81260983d*E (JD2415650 - 32800) TV Cas |[01926]. From photoelectric observations Min I = TV Cas |2432827.7665 + 1.8126142d*E (JD2432800 - 36490); TV Cas |Min I = 2436483.8091 + 1.81255d*E (JD2436480 - 36980); TV Cas |Min I = 2438472.2386 + 1.81263d*E (JD2437000 - 38500); TV Cas |Min I = 2438829.3230 + 1.8126048d*E (JD2438470 - 41750); TV Cas |since JD2441750 - see Table. TW Cas |Min II 8.40. TX Cas |Min II 9.6. TY Cas |P var. Max = 2419260 + 545.0d*E (JD2419200 - 25300); TY Cas |Max = 2428965 + 623.8d*E (JD2427000 - 41500); TY Cas |since JD2441500 - see Table. UU Cas |Min II 10.5. UZ Cas |[A/H] = -0.3. VV Cas |P var. Max = 2422514.16 + 6.207510d*E (JD2417000 - 32500); VV Cas |since JD2432500 - see Table. [A/H] = -0.2. VW Cas |[A/H] = 0.0. WY Cas |In the region of the cluster NGC 7789. WY Cas |The spectrum of the G type star is seen in minimum light WY Cas |[03502]. The existence of a physical companion is possible. WY Cas |S6/6-e. WZ Cas |VB A (optical companion B 8.7m, 58", 89deg). SC7/10e. WZ Cas |Light variations are sometimes taking place with doubled WZ Cas |period. XX Cas |Min II 10.2. YZ Cas |VB A (B 11.23m, 35", 160deg). d = 0.045P. Min II 5.78. ZZ Cas |Min II 10.9. AB Cas |EA/SD. Min II 10.28. P var. Min I = 2430755.678 + AB Cas |1.366863d*E (JD2425400 - 33150); Min I = AB Cas |2433616.532 + 1.366876d*E (JD2433150 - 37000); AB Cas |Min I = 2440475.5216 + 1.3668783d*E (JD2437000 - AB Cas |41600); since JD2441600 - see Table. AB Cas |The A3 component is a DSCT type variable with the elements: AB Cas |Max hel = 2444912.1759 + 0.0582874d*E [08825]; amplitude AB Cas |of pulsations Delta(V) var (0.03m <= Delta(V) <= 0.09m). AE Cas |Min II 12.8. AH Cas |Min II 13.3. AL Cas |Min II 13.6. AO Cas |Min II 6.24. The light curve shape var. P var? AQ Cas |Min II 10.4. AR Cas |VB A (B 9.3m, 1.0", 336deg; C 8.2m, 75", 269deg; AR Cas |D 9.8m, 76", 268deg; E 11.28m, 43", 115deg; F 11.06m, 69", AR Cas |338deg; G 11.11m, 67", 348deg). Min II 4.86; AR Cas |Min II - Min I = 0.614P; DII = 0.076P; dII = 0.037P. AS Cas |VB A (B 15.5m, 3", 45deg). AS Cas |Fundamental mode period P0 is given in the Table; the AS Cas |corresponding amplitude is 0.59m. First-overtone period AS Cas |P1 = 2.2909d; amplitude of oscillations with this period AS Cas |is 0.13m. P1/P0 = 0.76. AX Cas |Min II 12.9. AZ Cas |B - V: +1.78, +2.20. D = 110d, d = 88d = 0.026P. BD Cas |B - V: +1.50, +1.61. P var. Max = 2429124.84 + BD Cas |3.65129d*E (JD2415000 - 29130) [00915]; BD Cas |since JD2429130 - see Table. BE Cas |VB A (B G, 25", 260deg). BH Cas |According to [00453] there are no variable stars on the BH Cas |place of BH Cas and in its surroundings. BM Cas |Min II 8.98. Shape of the light curve varies. P var. BM Cas |There is a periodic term in the elements: BM Cas |+2.6d*sin(7.11deg*E + 104deg).According to [00939], on the BM Cas |light curve cepheid-like variations are observed with BM Cas |P = 27d. BN Cas |Min II 13.4. BS Cas |Min II 12.6. BU Cas |D = 0.02P. BY Cas |In the region of the cluster NGC 663. P var. BY Cas |Max = 2416871.91 + 3.2218d*E (JD2416800 - 24860) [00921]; BY Cas |Max = 2431929.60 + 3.221297d*E (JD2426900 - 34300); BY Cas |Max = 2438399.629 + 3.222588d*E (JD2436200 - 39400); BY Cas |since JD2439400 - see Table. BZ Cas |Min II 11.5. CC Cas |Min II 7.26. The light curve shape var? P var? CE CasA|Possible member of the cluster NGC 7790. VB A (B = CEb Cas, CE CasA|2.4", 265deg). CE CasB|VB B (A = CEa Cas). Possible member of the cluster NGC 7790. CF Cas |Possible member of the cluster NGC 7790. [A/H] = 0.1. CG Cas |In the region of the cluster NGC 7790. CH Cas |[A/H] = -0.5. CQ Cas |The slow oscillations are superimposed by more rapid ones CQ Cas |with cycles from 110d to 250d. CR Cas |Min II 13.3. CS Cas |[A/H] = -0.4. CV Cas |Epochs given in [00922] are not represented by the elements CV Cas |given in the Table. P var? CW Cas |Min II 11.47. Shape of the light curve and depths of CW Cas |minima vary. P var. Min I = 2435745.6163 + 0.31886497d*E CW Cas |(JD2432400 - 41000) [03332]; since JD2441000 - see Table. CY Cas |[A/H] = -0.7. DD Cas |P var. Max = 2415612.45 + 9.807272d*E (JD2415600 - 18600); DD Cas |since JD2418600 - see Table. The star may be a member of a DD Cas |binary system with Porb = 8500d +- 1000d. DF Cas |In the region of the cluster NGC 1027. DI Cas |P var. Max = 2432068 + 371.7d*E (JD2417200 - 32100); DI Cas |since JD2432100 - see Table. DL Cas |Member of the cluster NGC 129. [A/H] = 0.0. DN Cas |Min II 10.13. DO Cas |Min II 8.61; dI = 0.08P. DP Cas |Min II 13.6. DZ Cas |Min II 12.0. EG Cas |Min II 13.1. EK Cas |Depth of Min II 0.05m. EM Cas |P var. Max = 2433132 + 283d*E (JD2427700 - 33150); since EM Cas |JD2433150 - see Table. Amplitude strongly varies. EN Cas |Min II 12.4. P var. EP Cas |Min II 11.4. EQ Cas |Min II 12.7. P var. Min I = 2432150.04 + 58.26d*E EQ Cas |(JD2432200 - 34060) [03336]; since JD2436100 - see Table. EY Cas |Min II 14.5. GG Cas |d = 0.013P. Min II 9.99. P var? Min I = 2430188.468 + GG Cas |3.758738d*E (JD2424800 - 39500) [00936]; GG Cas |since JD2439500 - see Table. GK Cas |Depth of Min II 0.05m. GT Cas |d = 0.02P. GU Cas |Min II 11.3. P var. Min I = 2428749.423 + 3.093329d*E GU Cas |(JD2417470 - 35480) [00941]; GU Cas |Min I = 2437367.375 + 3.09325d*E (JD2435480 - 38750) [00001]; GU Cas |since JD2438750 - see Table. GZ Cas |Mean magnitude varies with P = 800d. GZ Cas |Max = 2428000 + 800d*E [00911]. HH Cas |Epoch of Min is given. RV type is possible [00911]. HN Cas |d = 0.038P. HS Cas |VB A (B 12m, 27", 15deg). HT Cas |Min hel = 2443727.93722 + 0.073647217d*E; HT Cas |D = 0.13P. Depth of eclipses between outbursts is ~2.4 V. HT Cas |Small quasi-periodic light oscillations with P = 100s. HT Cas |Spectrum description [06163]. HU Cas |P var. Max = 2417525.075 + 0.41159875d*E (JD2411600 - HU Cas |28000); since JD2428000 - see Table. IL Cas |Depth of Min II 0.05m. IR Cas |Min II 11.5. P var. Min I = 2428750.2914 + IR Cas |0.68069178d*E (JD2417500 - 38400) [00098]; IR Cas |since JD2438400 - see Table. IS Cas |Min II 12.2. P var. Min I = 2428776.262 + IS Cas |1.8415172d*E (JD2417400 - 29500) [00098]; IS Cas |since JD2428000 - see Table. IT Cas |Min II 11.8; Min II - Min I = 0.553P; DII = 0.042P. IT Cas |Apsidal motion is possible. IV Cas |Min II 11.3. P var. Min I = 2428991.302 + IV Cas |0.9985232d*E (JD2416700 - 29000) [00098]; IV Cas |Min I = 2431438.648 + 0.9985056d*E (JD2429000 - IV Cas |37700) [02263]; since JD2440000 - see Table. IW Cas |S4 +/6e. IX Cas |P var. Max = 2428749.39 + 9.15035d*E (JD2414700 - IX Cas |29500) [00098]; Max = 2428749.90 + 9.1363d*E IX Cas |(JD2428700 - 34350) [00944]; Max = 2437195.642 + IX Cas |9.14783d*E (JD2434350 - 39100) [05462]; IX Cas |since JD2442000 - see Table. [A/H] = -0.4. KL Cas |Min II 12.3. KO Cas |P var. Max = 2425590 + 305.6d*E (JD2416700 - 26000); KO Cas |since JD2426000 - see Table. KR Cas |Min II 9.9. LR Cas |Min II 10.9. LU Cas |Min II 14.3? LW Cas |In the apex of a small (8") bright cometary nebula in the LW Cas |region of IC 1848. Novalike outburst was observed in the LW Cas |interval JD2433900 - 34800. Infrared and radioemission. LX Cas |In the region of the cluster Collinder 33. Min II 15.3; LX Cas |Min II - Min I = 0.47P; dI = 0.10P. LY Cas |In the region of the cluster Collinder 33. Min II 15.2. MM Cas |d = 0.08P: Min II 12.4. MN Cas |Min II 10.57. MO Cas |In the nebula NGC 7635. 10.2 - 13.1 I. MP Cas |In the nebula NGC 7635. 10.4 - 13.5 I. MR Cas |Min II 15.5. MS Cas |Min II 13.2. MT Cas |d = 0.04P. Min II 14.02. MU Cas |Min II 10.8. MV Cas |Min II 14.0. MY Cas |Min II 15.2. P var. Elements given in the Table are valid MY Cas |since JD2438500. NN Cas |Min II 14.0. NT Cas |Min II 14.4. NU Cas |Min II 13.4. NV Cas |d = 0.03P. OP Cas |P var. Max = 2429109.726 + 5.510019d*E (JD2427950 - 34670) OP Cas |[00176]; since JD2437000 - see Table. OR Cas |Min II 11.8. P var. Min I = 2429249.424 + 1.2457026d*E OR Cas |(JD2413800 - 34800) [00176]; since JD2432000 - see Table. OX Cas |In the region of the cluster NGC 381. d = 0.016P. Min II OX Cas |10.30; Min II - Min I = 0.512P. Apsidal motion [04524]. PR Cas |P = 171d? PV Cas |Min II 10.36; Min II - Min I = 0.480P. PV Cas |Depth of Minima probably varies. P var. Min I = PV Cas |2428796.8142 + 1.75047346d*E (JD2415700 - 40000) [05302]; PV Cas |since JD2440000 - see Table. Apsidal motion [06253]: PV Cas |Min II = 2428797.6894 + 1.75047346d*E - PV Cas |0.040d*sin(0.0075deg*(E - 3000)). PX Cas |Min II 15.0. PY Cas |Epoch of Min brighness is given. Similar to RV Tau by PY Cas |light curve shape [03348]. PZ Cas |VB A (B 12.8m, WN 8:, 15", 100deg). OH, H2O emission. QQ Cas |Min II 10.8. P var. Min I = 2434330.169 + 2.142030d*E QQ Cas |(JD2415700 - 30000) [02530]; since JD2430000 - see Table. QX Cas |In the region of the cluster NGC 7790. VB A (B 13.1m, 3"). QX Cas |Min II 10.50; Min II - Min I = 0.37P; DII = 0.047P; QX Cas |dII = 0.018P. V0336 Cas |Min II 13.6. V0341 Cas |d = 0.031P. V0344 Cas |Min II 13.4. V0345 Cas |Min II 13.6. V0346 Cas |The coordinates refer to the sp component of a wide pair, V0346 Cas |whereas the chart [02345] leads to the nf component. It is V0346 Cas |the sp component that is red and probably var. V0357 Cas |Min II 13.6. V0359 Cas |Min II 12.0. V0360 Cas |Min II 12.3. V0361 Cas |d = 0.051P. V0363 Cas |Delta(S) = 1. V0364 Cas |Min II 11.9. V0365 Cas |S6/3- . V0366 Cas |Min II 12.7. P var. Min I = 2435075.461 + 0.7292714d*E V0366 Cas |(JD2414600 - 35400) [02305]; since JD2434650 - see Table. V0373 Cas |An unique close binary. Porb = 13.4192d [04627]. Epoch V0373 Cas |of Min I is given close to the epoch of one of V0373 Cas |conjunctions. Min II - Min I = 0.58P. Maxima are very V0373 Cas |sharp. Max - Min II = 0.25P. It is not excluded that the V0373 Cas |star is an eclipsing one with physical variability of V0373 Cas |components, but eclipses, if they exist, cause only a very V0373 Cas |small part of the observed light variations. Range of V0373 Cas |light variations is given according to [02651]. As a rule V0373 Cas |the amplitude is close to 0.1m. V0374 Cas |Min II 12.1. V0375 Cas |Min II 10.6. V0377 Cas |VB (A 8.5m; B 9.4m, 2.1", 185deg, 1962).It is not known V0377 Cas |which component varies. According to [04005] the range V0377 Cas |of combined brightness variations is 0.26m. V0377 Cas |According to [07051], const. V0380 Cas |d = 0.08P. V0381 Cas |Min II 10.8. V0388 Cas |Wolf 47 (mu = 0.82", p = 80deg). Faint component of a wide V0388 Cas |physical pair (p = 294") the bright component of V0388 Cas |which is the dM2 star Wolf 46 = BD+61deg 195 (9.4). V0392 Cas |Min II 14.0. P var. Min I = 2429640.390 + V0392 Cas |4.54094d*E (JD2425300 - 29640); Min I = V0392 Cas |2429640.390 + 4.54064d*E (JD2429640 - 36900) [04027]; V0392 Cas |since JD2436900 - see Table. Depth of Min var? V0394 Cas |Min II 15.6. V0396 Cas |Min II 10.2. V0399 Cas |Min II 14.1. V0401 Cas |Min II 15.7. V0402 Cas |Min II 15.3. V0406 Cas |Min II 16.8. V0410 Cas |Bright in 1938 -39. Slow. Not red. V0423 Cas |Min II 14.3. V0427 Cas |Min II 13.7. V0428 Cas |Red. V0430 Cas |Northern component of a close pair. Red. V0434 Cas |Red. V0441 Cas |P = 351.2d? V0442 Cas |d = 0.025P. P var? Since 1972 P = 3.592120d. V0444 Cas |Min II 16.0. P var. Min I = 2438651.314 + 2.224808d*E V0444 Cas |(JD2432850 - 37300); since JD2437300 - see Table. Period V0444 Cas |variation may be cyclic. Mean elements: V0444 Cas |Min I = 2443194.258 + 2.224773d*E. V0445 Cas |Min II 11.08. V0448 Cas |Min II 15.0. V0450 Cas |VB A (B 17.5m:, 3.4", 188deg). Range V0450 Cas |of combined light variations is given. V0459 Cas |Min II 11.6. V0466 Cas |In the region of the cluster NGC 457. V0480 Cas |Min II 14.7. V0482 Cas |VB A (B 10.0m, F 4 V, 6", 195deg; optical). P = 0.28292d? V0497 Cas |In the region of the cluster IC 1848. V0498 Cas |In the region of the cluster IC 1848. V0499 Cas |In the region of the cluster IC 1848. V0509 Cas |Pulsation of photosphere with P = 3 years. V0509 Cas |Tenuous shell ejected in 1975 is now falling back to V0509 Cas |the star. V0518 Cas |In the region of the cluster Stock 2. Star N136 (Stock 208). V0520 Cas |Min II 13.1. P var. Min I = 2439069.559 + 0.489832d*E V0520 Cas |(JD2438580 - 40850); since JD2441150 - see Table. V0521 Cas |Member of the cluster NGC 7789. V0523 Cas |Min II 11.34. P var. Min I = 2432054.555 + V0523 Cas |0.2336882d*E (JD2428545 - 33570) [07008]; V0523 Cas |Min I = 2439029.461 + 0.23368912d*E (JD2439000 - 41300) V0523 Cas |[07387]; since JD2440480 - see Table. V0524 Cas |OH, H2O emission. P = 163d?, 191d? 259d?, 620d? V0526 Cas |Two oscillations are superimposed: P1 = 0.0526d (A1 = V0526 Cas |0.0036m), P2 = 0.0396d (A2 = 0.0056m); P2/P1 = 0.753. V0527 Cas |Min II 13.5; Min II - Min I = 0.52P. V0532 Cas |In the region of the cluster NGC 7789. V0533 Cas |In the region of the cluster NGC 7789. V0536 Cas |P var. Max = 2438700.262 + 0.395674d*E V0536 Cas |(JD2438580 - 39150); Max = 2441186.333 + V0536 Cas |0.395683D*E (JD2440070 - 41250); V0536 Cas |since JD2441500 - see Table. V0540 Cas |Epoch of Max (U) is given. V0541 Cas |Min II 11.0. V0542 Cas |In the region of the cluster NGC 7789. V0544 Cas |Elements given in the Table are valid since JD2428000. V0546 Cas |In the region of the cluster NGC 103. Min II 14.8. V0547 Cas |VB A (B 12.4m, M4.5, 2.8", 93deg). Astrometric binary V0547 Cas |(A = 0.12", P = 15.9a); mu = 1.75", P = 98deg. V0547 Cas |Variation of combined light is given. V0551 Cas |P = 45.5d?/57d?/67.5d?. V0554 Cas |P >= 3500d? D = 400d? V0559 Cas |VB A (B 7.7m, 0.25", 34deg, 1976). Min II 7.21. V0566 Cas |VB A (B 8.3m, 1.4", 194deg, 1965). V0569 Cas |10.0 - 14.7 I. V0589 Cas |In the cluster NGC 663. V0592 Cas |White dwarf. Rapid non-periodic fluctuations of brightness V0592 Cas |on a time scale of several minutes. V0598 Cas |VB A (B 12m, 19", 0deg). P = 2.825d? [02560]. V0615 Cas |Variable radio source on 10.5 GHz; gamma - and X-ray V0615 Cas |source? V0627 Cas |H2O emission. V0635 Cas |4U 0115 + 634. SB (P = 24.3162d). V0635 Cas |Pulsar period P = 3.6136s. V0638 Cas |Epoch of Min is given. V0742 Cas |SB, Porb = 55.9212d. V0745 Cas |Component B of the double system observed brighter than in the V0745 Cas |Hipparcos Input Catalogue. V0746 Cas |SB, Porb = 27.8d. V0747 Cas |VB. The variability may be due to the fainter component. alf Cas |VB A (B 14.5m, 17.6", 272deg; C 13.5m, 38", 105deg; alf Cas |D 8.5m, 64.4", 280deg.) bet Cas |VB A (B 13.7m, 31.3", 243deg); SB (P = 27d). bet Cas |[Fe/H] = 0.64. gam Cas |VB A (B 11.0m, 2.2", 248deg; C 13.0m, 52.2", 348deg). gam Cas |In HII region S 185. X-ray source MX 0053 + 60. gam Cas |v sin i = 310 km/s. del Cas |VB A (B 11.5m, 31.7", 66deg). Min II 2.75. Min II - Min I = del Cas |361d. The elements given in the Table are still not del Cas |confirmed by anyone. iot Cas |VB A (B 6.89m, 2.3", 239deg; C 8.40m, 7.2", 114deg). iot Cas |Astrometric binary (a = 0.113", P = 52.4a). Max (V) - Max iot Cas |(lambda 1550) = 0.4P; A (lambda 1550) = 0.40m. The range iot Cas |of total brightness variation of components A and iot Cas |B is given. kap Cas |P = 0.09028d, P(Vr) = 0.14035d [02588]; P = 7d [08876]. omi Cas |VB A (B 11.7m, 33.6", 303deg). SB1 (P = 1033d); omi Cas |V sin I = 220 km/s. pi Cas |SB, Porb = 1.9642d. rho Cas |Usually varies within the limits 4.4m - 5.2m V. rho Cas |In November 1945 the peculiar decrease of brightness began rho Cas |lasting for 165d and in September 1946 the star reached rho Cas |the middle of the deepest minimum (JD2432070) lasting for rho Cas |320d. Then the brightness began to increase symmetrically rho Cas |and by July 1947 the star attained its normal brightness rho Cas |[00957]. Photographic magnitudes varied in the limits rho Cas |5.4m - 8.3m. Spectrum description [08878]. B Cas |Tycho Brahe's supernova. Stellar object is not identified B Cas |optically up to now. R Cen |VB A (B 12m, 28", 218deg). Epoch R Cen |of Min I is given. Min I 0.00P, Max I 0.23P, Min II R Cen |0.47P, Max II 0.64P. <Max I> 5.8, <Max II> 6.0, R Cen |<Min I> 11.1, <Min II> 8.3. P var. P = 561.3d R Cen |before 1918; since 1918 - see Table. H2O maser. V Cen |In the field of the open cluster NGC 5662. Z Cen |SN 1895 (NGC 5253). RR Cen |Min II 7.63. dII = 0.08P. P var. Min I = 2424231.0910 + RR Cen |0.60568807d*E + 2.31d*10**(-10)*E**2 (JD2414170 - RR Cen |33470) [00006]. Current elements - see Table. RS Cen |A 1118-61? RT Cen |P var. RZ Cen |Min II 9.4. SS Cen |Min II 9.5. ST Cen |Min II 11.30, DII = 0.22P. Max II (before ST Cen |Min I) 10.65. SU Cen |Min II 9.2. SV Cen |Min II 9.45. Delta(m) var. P var. Min = 2433053.358 + SV Cen |1.6594795d*E - 7.61d*10**(-8)*E**2 (JD2412608 - 42097). SV Cen |Cyclic (32a - 33.6a) period variations were noted in SV Cen |[00009,05212]. Since 1978 - see Table. P Cyg profiles in SV Cen |the spectrum. SX Cen |For mean light Max = 2426835 + 615d*E. SY Cen |d = 0.05P. SZ Cen |VB. Min II 8.7. TX Cen |VB? B - V: +1.39, +2.11. TZ Cen |The co-ordinates in the Table are based on [00015]. TZ Cen |According to [00016], no star brighter than 14m was found TZ Cen |in this position. The co-ordinates in [00015] may be in TZ Cen |error. UW Cen |IR excess.In Max varies semiregularly, P ~42d [08832]. UZ Cen |VB A (B 13.8m, 4", 191deg). Max II = 2440746.2 + UZ Cen |2.35529d*E. VW Cen |VB A (B ~15m?, ~8", ~180deg). B - V: +1.01, +1.71. VW Cen |[A/H] = 0.3. VZ Cen |Min II 8.4. WX Cen |<B - V> ~ +0.45, <U - B> ~ -0.72. WX Cen |Proposed as an optical counterpart of the transient X-ray WX Cen |source Cen X-2 [05314], though no optical bursts were WX Cen |observed. WZ Cen |Min II 14.2. ZZ Cen |VB C (A 9.4m, B9; B 10.8m, 8", 314deg; C = ZZ Cen, ZZ Cen |9", 259deg; D = AA Cen, 9", 110deg). AA Cen |VB D (see ZZ Cen). AB Cen |d = 0.05P. AP Cen |Epoch of Min is given. AS Cen |Min II 13.2. AV Cen |Min II 14.1. AZ Cen |The shape of the light curve varies. BD Cen |Min II 10.7. BF Cen |In the field of the open cluster NGC 3766. Min II 8.8. BG Cen |Min II 12.3. BH Cen |In the open cluster IC 2994. Min II 8.8. BI Cen |Delta(S) = 2. BK Cen |P2 = 2.236d, A1 = 0.54m, A2 = 0.22m [08835]. BV Cen |The mean cycle between outbursts <= 149.4d [07301]. The BV Cen |tabulated elements correspond to Max of the eclipsing BV Cen |light curve, phi (Min) = 0.25P. The range of the eclipsing BV Cen |variability is 12.8 - 13.3. CN Cen |Min II 13.3. DI Cen |Min II 12.3, Min II - Min I = 0.494P, DII = 0.08P:. DT Cen |Red. DX Cen |The P star in a pair. DY Cen |All spectral lines are very weak. No IR excess. The DY Cen |photometric behaviour outside major Min is described in DY Cen |[08836]. EP Cen |Min II 11.5. EU Cen |The P star in a pair. GI Cen |In the field of the globular cluster NGC 5286. GM Cen |The chart in [06286] is wrong. IQ Cen |d = 0.04P. IW Cen |Min II 12.1. IX Cen |In the field of the open cluster NGC 3706. IY Cen |In the field of the open cluster IC 2944. IZ Cen |<B - V> = 1.7. KK Cen |B - V: +1.08, +1.62. KM Cen |Min II 13.3. KN Cen |B - V: +1.36, +1.75. [A/H] = 0.2. KQ Cen |Alternating periods 136d, 159d. KT Cen |B - V: +0.46. Min II 12.72. Min II - Min I = 0.392P KT Cen |(JD2441686 - 721); apsidal motion is observed [08094]. KY Cen |Min II 13.3. KZ Cen |B - V: +0.30, +0.72. LL Cen |Min II 13.1. LR Cen |Min II 12.30. LT Cen |Min II 9.6. LU Cen |The period may be twice longer. LV Cen |B - V: +1.3, +1.7. LW Cen |Min II 9.6. In the field of the open cluster IC 2944. LX Cen |Min II 13.55. LZ Cen |Min II 8.50. MM Cen |Min II 12.7. MN Cen |Min II 8.7. VB A (B 10.9m, 7", 147deg). MP Cen |Min II 10.0. MQ Cen |Min II 10.1. MR Cen |Min II 10.5. MV Cen |Min II 14.6. MY Cen |B - V: +1.58, +1.94. NO Cen |Min II 14.2. NP Cen |Min II 10.2. NY Cen |Min II 11.9. OO Cen |<B - V> = 1.84. OP Cen |Min II 13.8. OU Cen |Min II 10.9. OV Cen |Min II 11.0. OX Cen |Min II 14.3. QS Cen |d = 0.03P. QT Cen |Min II 13.4. QY Cen |<B - V> = 2.16. QZ Cen |P var? The shape of the light curve varies? V0339 Cen |VB A (B ~13m, SP). B - V: +1.08, +1.47. V0343 Cen |Min II 13.5. V0344 Cen |Min II 12.3. V0346 Cen |In the field of the open cluster Stock 14. Min II 8.8. V0346 Cen |Min II = 2421966.835 + 6.32189d*E. V0348 Cen |d = 0.010P. V0349 Cen |Min II 14.5. V0350 Cen |Min II 10.3. Min II = 2430870.192 + 3.216906d*E. V0351 Cen |Epoch of Min is given. V0356 Cen |Min II 15.0. V0358 Cen |Epoch of Min is given. V0365 Cen |d = 0.040P. V0373 Cen |VB A (B ~4" np). V0377 Cen |d = 0.003P. V0379 Cen |Min II 8.9. V0380 Cen |Min II 10.0. V0383 Cen |Min II 13.6:, Min II - Min I = 0.609P. V0384 Cen |Min II 12.2. DII = 0.062P. Min II - Min I = 0.667P. V0385 Cen |Min II 13.0. V0388 Cen |Min II 15.7. V0399 Cen |d = 0.020P. Min II 13.1. V0405 Cen |P var, 30d - 40d. V0412 Cen |VB A (B 59", 266deg). V0419 Cen |P var. Max = 2428099.25 + 5.50713d*E (JD2428099 - 33573); V0419 Cen |since JD2434900 - see Table. V0420 Cen |B - V: +0.45, +0.97. P var. Nonlinear term: V0420 Cen |-0.000090d*E**2. V0427 Cen |Epoch of Min is given. V0436 Cen |SB (P = 0.0669d). Photometric P during supermaxima V0436 Cen |0.06383d [08838]. Rapid oscillations in supermaxima V0436 Cen |Delta(m) ~0.002m, P ~19.6s [08049]. V0440 Cen |d = 0.033P. Min II is possible. V0443 Cen |d = 0.025P. V0491 Cen |Very flat minima; close companion? V0495 Cen |d = 0.042P. Min II 10.6. Min II - Min I = 0.520P. V0496 Cen |Possible member of the open cluster NGC 4755. V0496 Cen |B - V: +1.02, +1.33. V0498 Cen |P may be twice shorter. V0499 Cen |(k - b)2 = 0.23. V0504 Cen |Semiregular variations (P1 ~130d, P2 ~411d) V0504 Cen |are also observed [08836]. V0506 Cen |The chart in [06286] is wrong. V0508 Cen |Min II 13.2. V0526 Cen |Delta(m) var. P var. Max = 2425707.540 + 0.56153d*E V0526 Cen |(1929 - 1930); during 1931 - 1940 - see Table. V0527 Cen |The chart in [06286] is wrong. V0532 Cen |Star 1 [09078]. X-ray source 3A 1431-409. V0544 Cen |2AS E 1440-39? [05962]. The chart in [06286] is wrong. V0545 Cen |Magnitude in Max var (12.6 - 14.5), P = 1800d? V0553 Cen |[Fe/H] = -0.1; [C/Fe] = +0.8. V0565 Cen |Min II 13.9. Type RR is not excluded (P = 0.238072d). V0574 Cen |sp star of a pair. V0577 Cen |According to improved coordinates, the star is actually in V0577 Cen |Hydra. V0585 Cen |Min II 13.0. V0592 Cen |Mean brightness var. V0593 Cen |Possible member of the open cluster Stock 16. Min II 11.2. V0594 Cen |V133 (omega Cen); non-member of the cluster. Min II 14.4. V0606 Cen |Min II 9.8. V0607 Cen |Min II 14.1. V0608 Cen |Min II 13.1. V0609 Cen |Min II 13.6. V0615 Cen |Min II 14.0. V0617 Cen |Min II 13.8:. V0619 Cen |In the field of the open cluster NGC 5316. V0621 Cen |d = 0.05P. V0624 Cen |Min II 14.9. V0625 Cen |Min II 15.0. V0627 Cen |d = 0.02P. V0628 Cen |Min II 13.2. V0630 Cen |Min II 14.2. d = 0.06P. V0635 Cen |Min II 13.9. V0636 Cen |Min II 8.8. V0644 Cen |During the faint phase in 1951 the shell spectrum was V0644 Cen |observed [02128]. Type E with a very long period is V0644 Cen |possible [06763]. V0645 Cen |Proxima Cen = alpha Cen C. mu = 3.809", P = 281.7deg. V0645 Cen |Soft X-ray source. V0646 Cen |d = 0.022P. Min II 9.1. V0662 Cen |P ~2.48d or 2.95d. V0672 Cen |Min II 11.4 - 11.6 (var). V0673 Cen |Depth of Min II 0.05m. V0674 Cen |Blazhko effect: Pi = 29.5d. 0.15P <= M - m <= 0.23P. V0676 Cen |Min II 12.5. V0677 Cen |Min II 11.6. V0678 Cen |Min II 10.6. V0679 Cen |9.8"p, 1.1"n from CPD -62deg 2167. V0679 Cen |The star is at the edge of a dark cloud in a bright nebula, V0679 Cen |a part of IC 2944, in the field of a very poor open V0679 Cen |cluster. Since 1950 till 1954 faded by 2.5m. Rather red. V0679 Cen |"Screening" by the edge of a dark nebula? V0682 Cen |IR excess. V0684 Cen |Depth of Min II 0.05m. V0685 Cen |Min II 9.5. V0686 Cen |RV type is not excluded. V0687 Cen |Min II 14.1. DII = 0.12P. Min II - Min I = 0.580P. V0688 Cen |Min II 12.7. V0689 Cen |Min II 12.1. V0690 Cen |Depth of Min II 0.03m. V0692 Cen |Min II 11.6. Min II - Min I = 0.481P. V0701 Cen |VB? d = 0.026P. Min II 9.1. V0704 Cen |IR excess. V0716 Cen |Min II 6.21. V0742 Cen |Min II 10.1. V0743 Cen |(k - b)2 = 0.20. Elements almost as well satisfactory: V0743 Cen |Max = 2439243.6465 + 0.10222560d*E. V0745 Cen |Min II 9.6. V0746 Cen |= V467 Cen. Marked as V467 Cen in the chart. V0747 Cen |Min II 10.05. V0748 Cen |B - V: +0.31, +1.21; U - B: -0.66, -0.21. d = 0.106P. V0748 Cen |Narrow Halpha emission. Outside eclipses shows variations V0748 Cen |by 0.05m - 0.1m during several days or several weeks V0748 Cen |(probably irregularly) [06968]. V0752 Cen |Min II 9.61. dI = dII = 0.047P. V0753 Cen |(k - b)2 = 0.20. In the field of the open cluster NGC 3960; V0753 Cen |probably non-member. Type DSCT is possible. V0754 Cen |Slight Min II. V0755 Cen |In the Coalsack. V0756 Cen |In the Coalsack. High excitation lines (OVII, OVIII, CV) V0756 Cen |are present in the spectrum. WR type is possible [07372]. V0757 Cen |Min II 8.6. V0758 Cen |d = 0.07P. Min II 9.15. V0759 Cen |Min II 7.56. V0761 Cen |IR excess. V0763 Cen |VB A (B 13m, 7", 163deg). V0766 Cen |VB A (B 10.01m, B0Ibp, 9", 318deg). IR excess. V0767 Cen |VB A (B 11.52m, 21", 350deg). V0768 Cen |Possible P: 60d - 80d. V0770 Cen |According to [07570], const? V0772 Cen |In the region of the open cluster IC 2944. V0775 Cen |EB type is possible. Deep Min II. V0777 Cen |Deep Min II. V0779 Cen |Cen X-3 (3U 1118-60). <B - V>: +1.04; <U - B>: -0.08. V0779 Cen |Min II 13.39. Porb var. The shape of the light curve V0779 Cen |varies. Epoch of Min I is given. Epochs of Min II coincide V0779 Cen |with the moments of X-ray eclipses. X-ray pulses are V0779 Cen |observed with Ppuls = 4.834477s (epoch JD2442785.3); V0779 Cen |Ppuls decreases [07612]. No rapid optical oscillations V0779 Cen |were found. V0783 Cen |B - V: +0.35. V0784 Cen |Very red. V0788 Cen |Min II 5.90. V0790 Cen |VB B (A 4.52m; 60", 343deg). V0791 Cen |In the region of globular cluster omega Cen (NGC 5139). V0791 Cen |Cluster non-member. V0795 Cen |VB A (B 12.29m, 33.9", 170deg; C 12.79m, 36", 220deg). V0801 Cen |4U 1145 - 61 = 2S 1145 - 619. Primary component has a low V0801 Cen |density envelope expanding with the velocity of 1800 km/s. V0801 Cen |V sin i = 290 km/s. X-ray pulsar (P = 291.8s V0801 Cen |[08883]). Max (X) = 2442519.5 + 187.5d*E [08881]. V0803 Cen |Extremely hot hydrogen-deficient helium star. V0807 Cen |VB (9.9m, 10.1m, 0.4", 258deg, 1931). V0807 Cen |It is not known which of the components varies. V0810 Cen |Member of the cluster Stock 14. V0813 Cen |In the region of globular cluster omega Cen (NGC 5139). V0813 Cen |V65 (NGC 5139). V0814 Cen |In the region of globular cluster omega Cen (NGC 5139). V0814 Cen |V78 (NGC 5139). Min II 14.165:. Primary V0814 Cen |component is probably intrinsically variable [08884]. V0816 Cen |Primary oscillation is superimposed by the oscillations V0816 Cen |with freguencies: F2 = 4.9229, F3 = 4.7343, F4 = 4.9317 V0816 Cen |[02591]. V0820 Cen |[Fe/H] = -2.5; Vr = +260 km/s. V0822 Cen |Cen X-4. V0825 Cen |In the region of globular cluster omega Cen (NGC 5139). V0825 Cen |Cluster non-member. V2 (NGC 5139). V0826 Cen |In the region of globular cluster omega Cen (NGC 5139). V0826 Cen |Cluster non-member. V129 (NGC 5139). V0902 Cen |VB, rho = 12". Variability may be spurious. V0915 Cen |The variability type is not quite consistent with the spectral V0915 Cen |type (B9II/III). V0921 Cen |High proper motion (LTT 4397) not confirmed by HIPPARCOS data. V0933 Cen |HIPPARCOS data contradict the luminosity class V. V1015 Cen |Variability type and luminosity class (III) do not agree. V1045 Cen |Background field star. bet Cen |VB A (B 4.1m, 1.3", 251deg, 1960). SB1 (P = 352d bet Cen |[08887]. Multiperiodicity; sometimes brightness is constant bet Cen |[08215]. Soft X-ray source. del Cen |VB A (B 4.8m, 68.6", 325deg; C 6.5m, 16.6", 227deg). eps Cen |VB A (B 13.0m, 36.0", 158deg). There is a secondary light eps Cen |oscillation with the amplitude of 0.0034m and elements: eps Cen |Max = 2441041.058 + 0.17696d*E. eta Cen |VB A (B 13.5m, 5.6", 270deg, 1897); SB? mu Cen |VB A (B 13.63m, 48", 128deg). omi 1 Cen |VB A (B 11.4m, 13.5", 125deg). T Cep |P var. Max = 2414252 + 386.05d*E (JD2406900 - 20490); T Cep |Max = 2431086 + 394.93d*E (JD2420490 - 32900); T Cep |Max = 2440262 + 379.22d*E (JD2432900 - 42200); since T Cep |JD2442200 Max = 2444171 + 392.7d*E. Mean value of the T Cep |period is given in the Table. SiO maser. U Cep |VB A (B 11.83m, 13.9", 62deg; C 12.3m, 23.0", 318deg). U Cep |0.010P <= d <= 0.040P. Min II 6.93. P var. Min I = U Cep |2407890.3346 + 2.4928551d*E + 5.15d*10**(-9)*E**2 U Cep |(JD2388855 - 2440790) [06468]; analysis of period U Cep |variations in this interval see also in [07395]; U Cep |Min I = 2441395.3604 + 2.4931048d*E (JD2440790 - 41600); U Cep |Min I = 2441679.5716 + 2.4930432d*E (JD2441600 - 950); U Cep |Min I = 2443753.7982 + 2.4930679d*E (JD2442100 - 43800); U Cep |since JD2444000 - see Table. Shape of the light curve U Cep |and depth of minima vary. Brightness of the secondary (G8) U Cep |varies sporadically. Subgiant brightening accompanies U Cep |eruptive mass transfer. The gaseous stream moving to the U Cep |primary (B7) component forms around it gaseous ring or U Cep |disc [08889]. W Cep |Slow oscillations with Pi ~2000d are superimposed by W Cep |oscillations with P ~350d. X Cep |OH emission? RS Cep |d = 0.039P. P var. Min = 2417140.469 + 12.419925d*E RS Cep |(JD2410000 - 31000) [02431]; since JD2431000 - see Table. RZ Cep |P var. Max = 2411640.654 + 0.308697d*E RZ Cep |(JD2411640 - 15000); Max = 2417144.620 + 0.3086203d*E RZ Cep |(JD2415600 - 20200); Max = 2421175.611 + RZ Cep |0.3086699d*E (JD2421175 - 23000); Max = RZ Cep |2423768.475 + 0.3086918d*E (JD2423000 - 31700); RZ Cep |Max = 2433768.493 + 0.3086383d*E (JD2433700 - RZ Cep |38300) [08890]; Max = 2438207.938 + 0.308645d*E RZ Cep |(JD2438200 - 39040) [03879]; Max = 2440834.579 + RZ Cep |0.3086735d*E (JD2440800 - 42640) [08890]; RZ Cep |since JD2442640 - see Table. Shape of the light curve and RZ Cep |the amplitude A vary with the Blazhko effect period RZ Cep |Pb = 96.8*P0 = 29.88d; Min A = 2441464.147 + 29.88d*N RZ Cep |[08891]. Long period variation of P0 with a period ~50 RZ Cep |years is possible. Delta(S) = 6. SS Cep |Mean brightness varies with cycles from some hundreds to SS Cep |thousands days. SU Cep |Min II 10.6. SV Cep |IR excess. SX Cep |In the region of the nebula NGC 7023. SY Cep |Min II 12.70. P var? SZ Cep |VB A (B 12.3m, 24.9", 263deg). S4/6e. TT Cep |VB A (B 17.0m, 8", 160deg). TY Cep |Epoch of Min I is given. UZ Cep |P var. Max = 2440969 + 297.68d*E (JD2414000 - 42000); UZ Cep |since JD2440000 - see Table. VV Cep |VB (0.05", 174deg, 1950)? 0.066P <= D <= 0.091P; VV Cep |0.040P <= d <= 0.077P. Depth of eclipses: 2.30m (lambda VV Cep |3500 A), 1.9m (U), 0.4m (B). M-component is of SRC type: VV Cep |Max = 2443045 + 118.37d*E [08698,08894]; A(V) <= 0.33m. VV Cep |Light oscillations are also noted with P ~58d [08895], VV Cep |25d and 150d [08896]. B-component may be also an intrinsic VV Cep |variable [02416]. Gaseous streams. Strong variable magnetic VV Cep |field. VW Cep |VB A (B 10.3m, a = 0.51", P = 30.45a [08897]); mu alpha = VW Cep |+0.0899s, mu delta = +0.560". Min II 7.56. VW Cep |Shape of the light curve and depths of Min I and Min II VW Cep |vary. P var. Min I = 2433483.4257 + 0.27831758d*E + VW Cep |0.050d*cos(0.004813deg*(E - 4700)) (JD2424763 - 41200) VW Cep |[06483]; since JD2441000 - see Table. Period VW Cep |change study see also in [08899]. X-ray source. VZ Cep |Min II 9.93. WX Cep |Min II 9.14; dI = 0.01P, dII = 0.00P. WY Cep |Min II 11.5. P var [02545]. WZ Cep |Min II 11.9. XX Cep |Min II 9.26. P var. Min I = 2425096.449 + 2.337340d*E XX Cep |(JD2414930 - 30000); Min I = 2441539.4917 + 2.3373059d*E XX Cep |(JD2430000 - 42300) [08902]. Since JD2441500 - see Table. XY Cep |Min II 10.10. P var? XZ Cep |Min II 8.43. ZZ Cep |VB A (B 10.2m, A2 P, 3.6", 202deg; C 10.87m, A5V, ZZ Cep |20.6", 219deg). Min II 8.74. AH Cep |Min II 7.03. Depth of minima varies. P var. AH Cep |Min I = 2434989.3702 + 1.7747274d*E (JD2415500 - 35000) AH Cep |[03604]; since JD2434900 - see Table: +3.12d*10**(-9)*E**2. AI Cep |Min II 9.48. AN Cep |Since JD2425200 primary and secondary maxima and minima AN Cep |appeared, and mean cycle became 254d. AV Cep |d <= 0.04P. BB Cep |d = 0.050P. BE Cep |Min II 13.0. BF Cep |P var. Max = 2437236 + 426.11d*E (JD2423600 - 37300); BF Cep |Max = 2441665 + 442.3d*E (JD2437300 - 42500); since BF Cep |JD2442500 - see Table. BH Cep |Sometimes strong Algol-like light weakenings are observed. BO Cep |Sometimes strong Algol-like light weakenings are observed. CO Cep |Min II 12.6; Min II - Min I = 0.552P; DII = 0.080P. CP Cep |P var? CQ Cep |Shape of the light curve and depth of minima vary. CQ Cep |According to [07401] on 1969 March 28/29 on the phase CQ Cep |0.56P a light decrease by 0.1m was observed and then a CQ Cep |rapid flare by 0.35m U, 0.13m B, 0.14m V. P var. Nonlinear CQ Cep |term: -10**(-9)*E**2. CR Cep |P var. Max = 2436846.94 + 6.23318d*E (JD2415000 - 30000) CR Cep |[03157]; since JD2430000 - see Table. CV Cep |S7/1.5. Mean brightness varies with a cycle ~2000d [00159]. CW Cep |VB A (B 12.29m, 20", 310deg). Min II 8.01; CW Cep |Min II - Min I = 0.478P (1972 yr). There is a sinusoidal CW Cep |term in the elements: +0.0250d*sin(0.0626deg*E - 28.3deg). CW Cep |Apsidal motion with P = 43a. CX Cep |Min II 12.16. CY Cep |Min II 16.5. DD Cep |P var. Max = 2427960 + 167.6d*E (JD2427900 - 30000); DD Cep |Max = 2429968 + 173.0d*E (JD2429900 - 33600); DD Cep |since JD2433600 - see Table. DH Cep |In the region of the cluster NGC 7380. Apsidal motion with DH Cep |P = 2.6a [00165]. DK Cep |Min II 12.4. DL Cep |Min II 12.7. DO Cep |VB B (A 9.87m, M4V; a = 2,4", P = 44.78a, e = 0.408); DO Cep |mu = 0.852", P = 242.6deg. DP Cep |Min II 14.4. DQ Cep |Multiperiodicity: P0 = 0.12420d: [08137], P1 = 0.061177d DQ Cep |[08914]. DX Cep |P var. Max = 2430603.712 + 0.5260395d*E (JD2415700 - 31000) DX Cep |[00001]; since JD2431000 - see Table. Delta(S) = 7. DY Cep |Min II 11.8. EE Cep |A var? EF Cep |Min II 12.6. P var? EG Cep |Min II 9.61. P var. Min I = 2439774.3322 + 0.54462091d*E EG Cep |(JD2415200 - 41000) [00001]; since JD2441000 - see Table. EH Cep |In the dark cloud near the diffuse nebula and the cluster EH Cep |NGC 7023. EI Cep |Min II 7.98. EK Cep |Min II 8.06; Min II - Min I = 0.545P (1965). Min II = EK Cep |2439022.8484 + 4.427797d*E [08160]. EK Cep |Apsidal motion (P = 4700a +- 600a) [08923]. EL Cep |P var. EM Cep |In the region of the cluster NGC 7160. VB A (a 12.8m, EM Cep |19.8", 281deg; B 7.9m, 62.5", 146deg). Min II 7.16. EM Cep |Shape of the light curve and depth of minima vary. EO Cep |Min II 12.3. EP Cep |In the cluster NGC 188. Min II 17.0. EQ Cep |In the cluster NGC 188. Min II 16.7. ER Cep |In the cluster NGC 188. Min II 16.27. ES Cep |In the cluster NGC 188. Min II 15.8. ES Cep |P var. Min I = 2439082.238 + 0.34468d*E (JD2438480 - 39090); ES Cep |Min I = 2439236.501 + 0.34264d*E (JD2439090 - 39280); ES Cep |Min I = 2439594.548 + 0.34250d*E (JD2439400 - 39600); ES Cep |since JD2439600 - see Table. A var. EX Cep |Min II 11.6. EY Cep |Min II 10.4. EZ Cep |P var. Max = 2416803.627 + 0.378990d*E (JD2415400 - 20000) EZ Cep |[00001]; since JD2420000 - see Table. FH Cep |Min II 12.1. FL Cep |d = 0.02P. FS Cep |Min II 12.0. FT Cep |VB A (B 18.3m, 5", 27deg). In the region of the diffuse FT Cep |nebula and the cluster NGC 7023. FU Cep |In the region of the diffuse nebula and the cluster FU Cep |NGC 7023. FV Cep |In the region of the diffuse nebula and the cluster FV Cep |NGC 7023. P = 0.4628d. FW Cep |In the region of the diffuse nebula and the cluster FW Cep |NGC 7023. GI Cep |Min II 11.9. GK Cep |Min II 7.35; dI = dII = 0.03P; Min II - Min I = 0.502P. GK Cep |P var. Min I = 2425189.526 + 0.9361614d*E GK Cep |(JD2415000 - 27500); Min I = 2438694.7070 + 0.9361714d*E GK Cep |(JD2427500 - 38200) [00001]; since JD2438200 - see Table. GL Cep |In the region of the diffuse nebula IC 1396 and the GL Cep |cluster Tr 37. GM Cep |In the region of the diffuse nebula IC 1396 and the GM Cep |cluster Tr 37. GP Cep |In the region of the HII zone S 132. Quadruple system, GP Cep |consisting of a WN6 + O8-B0III: eclipsing pair GP Cep |(P = 6.6883d) physically associated with an O + O pair GP Cep |(P = 3.4698d); the latter pair may be also an eclipsing GP Cep |or ellipsoidal variable [08931]. GS Cep |Min II 10.6. GT Cep |Min II 8.6. GW Cep |Min II 12.00. HK Cep |Min II 14.4. HZ Cep |In the region of the diffuse nebula and the cluster HZ Cep |NGC 7023. IL Cep |VB A (B 11.91m, 7", 326deg); P = 2.802d? IM Cep |Min II 13.6. IO Cep |Min II 11.7. IP Cep |Min II 12.1. IR Cep |VB (Delta(m) ~0.0m, 0.0" -0.2"). P var. IR Cep |Max = 2431060.878 + 2.114016d*E (JD2428335 - 31060) [00001]; IR Cep |since JD2440900 - see Table. IV Cep |VB B (A 16m; B 2.1", 191deg). IW Cep |Min II 13.7; Min II - Min I = 0.52P. IX Cep |d = 0.03P. Min II 17.0. KL Cep |d = 0.019P. KP Cep |Depth of Min II 0.03m. KV Cep |Min II 14.3. KY Cep |Flare with 65 sec duration. There is a blue object on the KY Cep |place of the flare [00001]. KZ Cep |VB (8.6m, 8.6m; 1.9", 348deg). Depths of spectral lines KZ Cep |vary: P = 0.212938d [06488]. LL Cep |Min II 14.0. LM Cep |Min II 12.8. LP Cep |Min II 13.8; Min II - Min I = 0.55P. LQ Cep |Eastern component of a double star. LU Cep |VB. LW Cep |Depth of Min II 0.05m. LZ Cep |Min II 5.63. In the Table: P(Vr) [04627]. MN Cep |Depth of Min II 0.08m? MQ Cep |Min II 15.7. MT Cep |Min II 15.5. MX Cep |SB (P = 16.03d) [08947]. MY Cep |In the cluster NGC 7419. Emission OH, H2O. MZ Cep |In the region of the cluster NGC 7419. NN Cep |Min II 8.52. NR Cep |Min II 13.6; d = 0.025P? NS Cep |Depth of Min II 0.04m. NW Cep |Preceding component of a close VB. Min II 10.7. NY Cep |VB A (B 10.33m, 10", 190deg); d = 0.003P; SB2, e = 0.49; NY Cep |Delta(gamma) = gamma2 - gamma1 = 32 km/s [07412]. OS Cep |Very red. OT Cep |Min II 13.3. OZ Cep |Red. PS Cep |In the region of the cluster NGC 7380. SB2 (P = 2.09168d) PS Cep |[05479]. PV Cep |In the dark cloud near the diffuse nebula and the cluster PV Cep |NGC 7023. At the apex of the bright variable fan nebula. PW Cep |In the region of the diffuse nebular and the cluster PW Cep |NGC 7023. QZ Cep |The map of surroundings given in [04015] for BV 323 is in QZ Cep |reality the map for BV 324 = QZ Cep. Min II 11.9. V0338 Cep |Min II 9.52. V0342 Cep |B - V = +3.6. V0344 Cep |B - V = +4.4. V0345 Cep |B - V = +5.0. V0346 Cep |B - V = +4.6. V0347 Cep |B - V = +4.5. V0351 Cep |VB A (B 13m, 20", 135deg). P var. Max = 2430615.57 + V0351 Cep |2.80511d*E (JD2429160 - 34300); Max = 2435749.12 + V0351 Cep |12.80556d*E (JD2435310 - 40885) [02830]. Since V0351 Cep |JD2442020 - see Table. V0421 Cep |SB, Porb1 = 5.4136d, Porb2 = 225.44d. V0447 Cep |The variability may be due to the fainter (B) component. V0448 Cep |SB, Porb = 7.7320d. V0453 Cep |SB, Porb = 54.723d. V0454 Cep |SB, Porb = 5.6556d. V0711 Cep |Variability refers to combined brightness of two nearly equal V0711 Cep |components at 5" separation. bet Cep |VB A (A 6m, 0.204", 47.2deg, 1977.9; B 7.84m, A2V, 13.6", bet Cep |250deg). SB1 (Porb = 10.893d) [06486]. P var. bet Cep |Max(Vr) = 2417359.715 + 0.1904795d*E (JD2415750 - 22000); bet Cep |Max(Vr) = 2422203.790 + 0.1904844d*E + bet Cep |2.9440d*10**(-11)*E**2 + 3.2671d*10**(-17)*E**3 bet Cep |(JD2422000 - 42630) [00177]. Elements given in the Table bet Cep |satisfy observations in 1967 - 69. del Cep |VB A (B 13.0m, 20.0", 285deg; C 6.10m - 6.37m, B7IV, del Cep |41.0", 191deg. P var. Max = 2393659.856 + 5.366438d*E del Cep |(JD2372200 - 96900); Max = 2413960.73 + 5.366386d*E del Cep |(JD2396900 - 2414050); since JD2414050 - see Table. del Cep |All observations in the interval JD2373090 - 45000 are del Cep |well represented also by the elements with a square term: del Cep |Max = 2442756.490 + 5.366270d*E - 7d*6*10**(-9)*E**2 del Cep |[08632]. eps Cep |VB A (B 9.5m, 127.8", 15deg, 1918). eps Cep |Multiperiodicity: P2 = 0.068073d eps Cep |(A2/2 = 0.0061m), P3 = 0.011823d? (A3/2 = 0.0022m); eps Cep |A1/2 = 0.0079m. zet Cep |Radial velocity varies. mu Cep |VB A (B 12.3m, 19.4", 262deg; C 12.7m, 41", 299deg). mu Cep |There is also the cycle with 4400d duration [08957]. W Cet |S5.5/2e. RR Cet |[Fe/H] = -1.26. P var. During JD2417500 - 28820 RR Cet |Max = 2417501.444 + 0.55302577d*E; since JD2433180 - see RR Cet |Table. According to [08726], the graph of O - C deviations RR Cet |from the elements given in [03506] is approximately RR Cet |sinusoidal, with Pi = 2600d and the amplitude 0.025d. RU Cet |(k - b)2 = 0.01. Delta(m) var? P var [02455]. Max = RU Cet |2426964.019 + 0.5863003d*E (JD2426500 - 28430) RU Cet |[00181]; Max = 2434143.056 + 0.5862676d*E RU Cet |(JD2433100 - 35820) [02431]; since JD2435820 - see Table. RV Cet |Delta(S) = 9. RW Cet |Min II 10.5. P var. During JD2426500 - 41000 RW Cet |Max = 2426585.503 + 0.9751814d*E [00001]; since RW Cet |JD2441000 - see Table. RX Cet |Delta(S) = 5. P var. Before JD2428500 Max = RX Cet |2425938.271 + 0.5737100d*E [03506]; since RX Cet |JD2430000 - see Table. RZ Cet |Delta(S) = 6.7. P var. During JD2426585 - 28630 RZ Cet |Max = 2426585.448 + 0.510633d*E [03506]; current RZ Cet |elements - see Table. SS Cet |d = 0.025P. P var. Min = 2429321.250 + 2.9739509d*E SS Cet |(JD2427340 - 30700) [02419]; Min = 2430698.160 + SS Cet |2.973992d*E (JD2429300 - 36650) [03115]; SS Cet |since JD2440000 - see Table. SV Cet |Min II 14.9. TT Cet |Min II 11.1. TU Cet |D = 0.043P. Min II 10.9. Min II - Min I = 0.478P. TU Cet |According to [03564], the spectrum is K2. TV Cet |Min II 9.10. DII = 0.03P. Min II - Min I = 0.494P. TW Cet |Min II 11.14. P var. Min I = 2430965.595 + TW Cet |0.316852d*E (JD2427650 - 31000) [00192]; Min I = TW Cet |2433611.3121 + 0.316846d*E (JD2433530 - 615) TW Cet |[00001]; since JD2440000 - see Table. TX Cet |B - V: +0.34, +0.37. Min II 11.12. TY Cet |Min II 12.1. UU Cet |(k - b)2 = 0.08. P var. Blazhko effect? UV Cet |VB B (A 12.45m, dM5.5e; a = 2.1", P = 25a). VV Cet |Min II 11.0. EB type is also possible. RR type with twice VV Cet |shorter period is not excluded. VX Cet |d = 0.026P. VY Cet |Min II 11.70. VZ Cet |ADS 1778 B (B 0.61", 122deg; A = omicron Cet). VZ Cet |Small variations are also observed on the time scale of VZ Cet |several hours, with superimposed 10 - 15 minute variations VZ Cet |and rare flares of approximately 2 minute duration VZ Cet |[06492]. A possible white dwarf with an accretion VZ Cet |disc [08926]. WW Cet |VR var (P = 0.160d) [04712]. WW Cet |Rapid oscillations (~10 min) of brightness are observed WW Cet |[04709]. WZ Cet |Min II 11.0. XY Cet |d = 0.02P. Min II 9.34. YY Cet |Min II 9.2. ZZ Cet |4 stable oscillations are observed simultaneously: ZZ Cet |P1 = 213.132605s, P2 = 212.768427s, P3 = 274.250814s, ZZ Cet |P4 = 274.774562s. AA Cet |ADS 1581 A (B 7.7m vis, SB 2, F5, 8.5", 304deg). AA Cet |Min II 6.7:. dII = 0.065P. AB Cet |ADS 1849 A (B 9.30m, 12", 293deg). SB? (VR var, AB Cet |P = 2.997814d). The period of magnetic variations is AB Cet |15.9d [08932]. AD Cet |ADS 180 A (B 10m, 3", 4deg). CL Cet |Type ELL: is also possible. EE Cet |The variability may be due to the fainter (B) component. EL Cet |SB2. del Cet |Nonlinear term: +2.20d*10**(-11)*E**2. omi Cet |ADS 1778 A (B = VZ Cet, 0.61", 122deg). Maser omi Cet |SiO, OH, H2O. S Cha |VB A (B 9.29m, 23", 134deg). T Cha |Occasionally quasiperiodic light changes are observed with T Cha |periods 3.2323d, 3.4375d, 4.1800d, 3.2436d operating T Cha |during 6 - 26 cycles. IR excess. Z Cha |VB A (B 5.6"). Eclipses: Min = Z Cha |2440264.68232 + 0.0744992195d*E + 7.88d*10**(-13)*E**2 Z Cha |[08938]. D = 0.065P; d = 0.026P. Depth of Min: Z Cha |1.73m - 2.11m B before the eclipse; 1.38m - 1.97m B after Z Cha |the eclipse. Periodic variations during Min light [07000]. Z Cha |Variations with P = 27.7s during a supermaximum [08049]. RS Cha |EA/DM. Min II 6.53. One of the components is a pulsating RS Cha |variable of DSCT type. P is in the range from 0.074d RS Cha |to 0.097d [08403]. Delta(M) = 0.01m - 0.03m in the combined RS Cha |light. RW Cha |Min II 14.6. RY Cha |Min II 14.0. RZ Cha |Min II 8.8. DII = 0.11P. SY Cha |Quasiperiodic variations were observed. (P = 6.2d [04305], SY Cha |P = 7.6d [08946]). TW Cha |Quasiperiodic variations (P = 8.68d [04462]). VW Cha |IR excess. VZ Cha |Quasiperiodic variations (P = 7.27d). YZ Cha |Delta(m) (Min II) = 0.4m. CG Cha |Min II 14.4. CH Cha |Min II 15.1. CX Cha |Min II 15.5. Uncertain elements. CY Cha |Min II 14.0. CZ Cha |Min II 14.6. DD Cha |Min II 14.7. DG Cha |Min II 14.5. zet Cha |SB. S Cir |Min II 10.9. T Cir |Min II 9.4. U Cir |P var. Before JD2417000 Max = 2412560 + 151d*E. V Cir |Min II 11.0. According to [00210], varies in the range V Cir |10.8m - 13.0m pg. W Cir |Found in Lupus, in 4deg to the north from the position W Cir |published by the discoverer [00211]. TW Cir |Min II 13.3. UY Cir |Red. UZ Cir |Epoch of main Max is given. Resembles R Cen. UZ Cir |Max I - Max II = 160d. VX Cir |P var. Before JD2418000 Max = 2414360 + 427d*E. AQ Cir |Possibly EW type with twice longer period. AR Cir |The magnitude in Min light possibly corresponds to an AR Cir |unresolved companion. AT Cir |d = 0.02d:. AX Cir |SB. VB? (6.5m; 6.5m; 0.5", 143deg, 1913). BD Cir |Min II 9.5. BF Cir |Min II 8.9. BG Cir |Min II 10.3. BN Cir |Deep Min II. Twice shorter period is not excluded. BR Cir |Cir X-1. According to [08951], the object does not coincide BR Cir |with the star (B = 22.5m) labelled as L in the chart in BR Cir |[02911] but is situated in ~1" to the south of it and has BR Cir |M > 23.5m on IIIa-J plates. Gradual increase of X-ray BR Cir |intensity is periodically stopped by an abrupt intensity BR Cir |fall. The moments of such transitions T are represented by BR Cir |the elements T = 2443292.118 + 16.595d*E [02926]. The X-ray BR Cir |intensity falls are accompanied by IR and radio bursts. BR Cir |Vr (e alpha) = +250 km/s. In 25' from the supernova BR Cir |remnant G 321.9-0.3. tet Cir |VB (6.2m, 6.2m, 0.1", 96deg). T Col |SiO maser. U Col |Min II 10.5. Y Col |V2 (NGC 1851). Z Col |V1 (NGC 1851). RS Col |Min II 9.97. dII = 0.021P. RY Col |(k - b)2 = 0.10. P var; nonlinear term: -3.38*10**(9)E**2. RZ Col |Min II 11.20. VW Col |Variability may be due to component B. TV Col |2A 0526 - 328. VB A (B 15.79m, 10", 330deg). Epoch of Max TV Col |of short-term photometric variations is given. The TV Col |following elements describe, respectively, moments of Max TV Col |Vr for Balmer lines and moments of Max for the TV Col |comparatively long-term photometric variations which are TV Col |due to the beat phenomenon for the photometric and TV Col |spectral periods: Max Vr = 2444227.631 + 0.228600d*E; TV Col |Max = 2444191.5 + 4.024d*E. Flickering up to 0.15m B and TV Col |flares up to 0.3m U are also observed [08960]. R Com |OH emission. S Com |Delta(S) = 8. T Com |OH, H2O emission. U Com |Delta(S) = 5. V Com |P var. Max = 2424518.219 + 0.46913844d*E V Com |(JD2420900 - 26900) [00218]; since JD2438100 - see Table. V Com |Delta(S) = 8. W Com |Radio source ON 231. X Com |Z = 0.092. Spectrum description [07415,08966]. Y Com |In the region of the globular cluster M 53 (NGC 5024). Z Com |In the region of the globular cluster M 53 (NGC 5024). RR Com |In the region of the globular cluster M 53 (NGC 5024). RS Com |In the region of the globular cluster NGC 5053. RT Com |In the region of the globular cluster NGC 5053. A var; RT Com |P var. Max = 2423113.496 + 0.5651925d*E (JD2422700 - RT Com |26450) [00222]; since JD2438535 - see Table. RU Com |In the region of the globular cluster M 53 (NGC 5024). RV Com |In the region of the globular cluster M 53 (NGC 5024). RW Com |In the region of the Comae Berenices cluster. dI = 0.04P; RW Com |Min II 11.56. P var. RW Com |Min I = 2433040.406 + 0.23734705d*E (JD2419680 - 34550) RW Com |[00185]; since JD2439600 - see Table. RY Com |P var. Max = 2425007.450 + 0.46894835d*E (JD2425000 - RY Com |27500) [03506]; Max = 2432674.390 + 0.4689397d*E RY Com |(JD2432600 - 38110) [03415]; since JD2438100 - see Table. RY Com |(k - b)2 = 0.07. RZ Com |Possible member of the Comae Berenices cluster. Min II RZ Com |11.09; dI = 0.043P, dII = 0.039P. P var. RZ Com |Min I = 2433396.737 + 0.33850556d*E (JD2425000 - 33300) RZ Com |[00226]; since JD2433300 - see Table. RZ Com |Shape of the light curve varies. SS Com |Min II 11.9. ST Com |Delta(S) = 10. SX Com |In the region of the globular cluster NGC 4147. SZ Com |In the region of the globular cluster NGC 4147. TU Com |Shape of the light curve, A and P vary. Mean elements TU Com |are given in the Table. Possible period of Blazhko effect TU Com |is 75d [03584]. [Fe/H] = -1.43. UU Com |Member of the Comae Berenices cluster. Light variations UU Com |are due to rotation and pulsations of the star. Rotational UU Com |period is 2.1953d or 1.0256d or 0.9178d. Period of UU Com |pulsations is 0.0227d (A ~0.01m). According to [07985] UU Com |there are two periods of pulsations: P1 = 0.0274d and UU Com |P2 = 0.0209d UU Com |(P2/P1 = 0.76). UV Com |[Fe/H] = -1.44. UW Com |[Fe/H] = -1.22. UX Com |Min II 10.13. P var; nonlinear term: -3.75d*10**(-8)*E**2. UY Com |[Fe/H] = -1.51. UZ Com |[Fe/H] = -1.44. VV Com |[Fe/H] = -1.53. VW Com |VB (12.00m, dM 3.5e; 12.3m, dM 4e, 3.0", 23deg, 1945). VW Com |Range of total brightness variation VW Com |is given. According to [08363] the component B is VW Com |variable. However both components may be variables. VY Com |Min II 14.5. AI Com |Member of the Comae Berenices cluster. VB A (B 6.63m, AI Com |145", 251deg). Pulsations are possible: P = 0.052d AI Com |(A = 0.02m) [08975]. AL Com |Within 8' to the south-east from the nucleus of M 88 AL Com |(NGC 4501) galaxy. AQ Com |Min II 15.7. BM Com |Min II 13.8. BS Com |P var. Max = 2434453.31 + 0.36341d*E (JD2434130 - 35230); BS Com |since JD2435590 - see Table. Shape of the light curve BS Com |varies. BZ Com |[Fe/H] = -1.21. CC Com |In the region of the Comae Berenices cluster. Min II CC Com |12.09; dI = 0.03P. CD Com |[Fe/H] = -1.78. CF Com |Shape of the light curve varies. CG Com |[Fe/H] = -1.06. CI Com |RRC? CK Com |P var. Max = 2437370.71 + 0.6940159d*E (JD2437370 - 40130); CK Com |Max = 2441630.35 + 0.6939080d*E (JD2440130 - 41630); CK Com |since JD2441630 - see Table. Blazhko effect. CK Com |[Fe/H] = -1.68. CL Com |[Fe/H] = -1.00. CN Com |Min II 13.5. CP Com |[Fe/H] = -1.19. CT Com |In the region of the Comae Berenices cluster. CV Com |In the region of the Comae Berenices cluster. CX Com |In the region of the Comae Berenices cluster. Not member CX Com |of the cluster. DD Com |Min II 14.90. DG Com |Min II 14.6. DL Com |P var? DR Com |EW? P = 0.45184d? DS Com |[Fe/H] = -1.32. DT Com |[Fe/H] = -1.60. DU Com |[Fe/H] = -1.45. DV Com |[Fe/H] = -1.57. DW Com |[Fe/H] = -1.53. EE Com |P = 0.539533d also satisfies observations. [Fe/H] = -1.64. EF Com |[Fe/H] = -1.90. EG Com |[Fe/H] = -1.29. EI Com |[Fe/H] = -1.68. EL Com |P = 0.52362d also satisfies observations. EM Com |[Fe/H] = -1.64. EN Com |[Fe/H] = -1.19. EO Com |[Fe/H] = -1.51. EP Com |[Fe/H] = -0.98. EQ Com |Min II 15.3. ER Com |[Fe/H] = -1.51. ES Com |[Fe/H] = -2.02. EW Com |[Fe/H] = -1.77. EX Com |P = 0.558359d? [Fe/H] = -1.48. EY Com |Min II 18.0. EZ Com |P = 0.568349d? [Fe/H] = -1.16. FG Com |P = 0.3098d also satisfies observations. FK Com |Wide emission lines, Halpha and H, K CaII, of variable FK Com |intensity. Epoch of light minimum is given. FM Com |The member of the Comae Berenices cluster. Multiperiodicity. FM Com |Cycle of 0.0713d was observed also [08989]. FO Com |In the region of the Comae Berenices cluster. FP Com |In the region of the Comae Berenices cluster. mu = 0.23", FP Com |P = 158deg. Red. FZ Com |P = 4.704864d? GM Com |In the region of the Comae Berenices cluster. GN Com |Member of the Comae Berenices cluster. P > 1d. GO Com |In the region of the Comae Berenices cluster. GP Com |mu = 0.38", p = 286deg. SB (Porb = 0.032306d). GP Com |Unique object G 61-29. Consists of two interacting white GP Com |dwarfs. The lower mass star, a helium white dwarf, GP Com |transfers mass to the higher mass star surrounded by an GP Com |accretion disk. Usually flares are being observed with an GP Com |amplitude about 0.2m V, 0.5m U lasting about 20 seconds GP Com |[07417,08991]. Sometimes periods of photometric activity GP Com |arise when amplitude of light variations reaches 0.6m V GP Com |and sharp passages from maxima to minima are being GP Com |observed; the duration of these minima reaches up to 0.14d GP Com |[07417]. When the star is most active, periodic light GP Com |oscillations appear with P = 105 seconds and amplitude GP Com |0.05m - 0.10m V [07062]. GQ Com |Z = 0.165. Emission H, [OIII]. Irregular light variations. GQ Com |<B - V> = +0.16. GT Com |Minor planet (679) Pax. HH Com |Epoch of Min in V system is given. HI Com |In the region of the Comae Berenices cluster. HK Com |In the region of the Comae Berenices cluster. HM Com |In the region of the Comae Berenices cluster. HN Com |In the region of the Comae Berenices cluster. HO Com |In the region of the Comae Berenices cluster. HP Com |In the region of the Comae Berenices cluster. HQ Com |In the region of the Comae Berenices cluster. HR Com |In the region of the Comae Berenices cluster. HS Com |In the region of the Comae Berenices cluster. HT Com |In the region of the Comae Berenices cluster. HU Com |In the region of the Comae Berenices cluster. HV Com |In the region of the Comae Berenices cluster. HW Com |In the region of the Comae Berenices cluster. R CrA |In the head of the bright cometary nebula NGC 6729. R CrA |IR excess. S CrA |VB A (B 13.5m, 1", 137deg). IR excess. T CrA |In the bright cometary nebula NGC 6729. IR excess. V CrA |Quasiperiodic variations (P ~75d, Delta(V) ~ 0.2m - 0.9m). V CrA |IR excess. RS CrA |sp of two close stars; each of them or both may be RS CrA |identified with CoD -39deg 13082. RW CrA |Min II 9.4. SS CrA |V1 (NGC 6541). SV CrA |The period may be twice shorter. TY CrA |VB A (B 13.3m, 4", 138deg; C 58", 24deg). TY CrA |In the bright nebula NGC 6726/27. P = 1.92d is not TY CrA |excluded, in that case Min II = Min I. On the basis of TY CrA |visual observations 8.7 - 12.4 v (presumably "spurious TY CrA |variability" due to the difficulties of estimates over TY CrA |the bright background of the nebula), and the star TY CrA |was classified as INSA. TZ CrA |Min II 9.72. UU CrA |Min II 11.0. UX CrA |The period may be twice shorter. UY CrA |P var? VV CrA |In the region of the bright nebula NGC 6729. IR excess. AF CrA |P var. Before JD2418060 Max = 2413710 + 483d*E; since AF CrA |JD2418060 - see Table. AL CrA |B - V: +0.65, +1.30. [A/H] = -0.2. AN CrA |P var. Nonlinear term: -0.006d*10**(-6)*E**2. AU CrA |P var. Nonlinear term: -0.026d*10**(-6)*E**2. AY CrA |Min II 15.2. BG CrA |Min II 15.1. BH CrA |P var. Nonlinear term: -0.023d*10**(-6)*E**2. CM CrA |P var. Nonlinear term: -0.007d*10**(-6)*E**2. CR CrA |Min II 15.7. CS CrA |Min II 15.2. CY CrA |P var. Nonlinear term: -0.002d*10**(-6)*E**2. DG CrA |In the region of the bright nebula NGC 6729. IR excess. DL CrA |Min II 13.6. DN CrA |P var. Nonlinear term: +0.006d*10**(-6)*E**2. DZ CrA |d = 0.02P. EE CrA |<mpg> var, 13.5m - 15.5m, P2 = 3000d - 5000d EE CrA |Delta(m) (P1 = 167d) ~1.5m. EK CrA |P var. Before JD2422600 Max = 2411870 + 421d*E. FF CrA |Before JD2423000 Max = 2411530 + 140.2d*E. FK CrA |Min II 14.5. FS CrA |Min II 14.5. FW CrA |Before JD2416600 Max = 2411190 + 112.2d*E. GS CrA |Before JD2422600 Max = 2414070 + 284d*E. IT CrA |Min II 13.6. KM CrA |The chart in [06286] is wrong. KQ CrA |[A/H] = -0.7. B - V: +0.76, +1.23. KT CrA |Red. LU CrA |P = 182d is possible. MS CrA |Yellow. MT CrA |Min II 13.1. NO CrA |Reddish. QR CrA |Reddish. V0347 CrA |B - V: +0.82, +1.17. V0350 CrA |Min II 13.4. V0385 CrA |The period may be spurious. V0413 CrA |(k - b)2 = 0.11. V0428 CrA |The period may be twice shorter. V0449 CrA |[A/H] = -0.3. V0454 CrA |Min II 10.5. V0455 CrA |d = 0.05P. Min II 13.7. V0457 CrA |Epoch of Min is given. EW type is also possible, in that V0457 CrA |case the value of P should be doubled. V0465 CrA |Min II 14.2. V0467 CrA |P var? V0471 CrA |Min II 13.3. V0478 CrA |Sometimes a cycle 60d - 70d. V0480 CrA |Min II 13.9. V0490 CrA |P var? The elements represent the observations of 1944. V0493 CrA |P var? V0501 CrA |Min II 13.4. Twice shorter period is possible. V0503 CrA |d = 0.03P. V0511 CrA |Twice longer period is possible. V0512 CrA |P var? V0513 CrA |Min II 13.2. V0514 CrA |Min II 14.0. V0527 CrA |P var. V0535 CrA |P var. V0541 CrA |P var? V0545 CrA |VB. Combined brightness with a faint companion is given. V0553 CrA |P var? V0566 CrA |Min II 12.7. V0568 CrA |Sometimes a cycle 60d - 80d. V0569 CrA |Min II 13.1. EB type is possible. V0571 CrA |Min II 14.7. V0572 CrA |Min II 14.0. V0577 CrA |Min II 13.2. RR type with twice shorter period is possible. V0578 CrA |RV type with P = 118d is possible. V0580 CrA |Min II 14.4. V0595 CrA |P var. V0601 CrA |Epoch of min is given. V0603 CrA |Slightly noticeable Min II at the phase 0.5P. V0604 CrA |d = 0.03P. V0607 CrA |Min II 14.3. V0612 CrA |d = 0.03P. V0615 CrA |P var? V0622 CrA |Sometimes 55d - 60d cycles. V0633 CrA |P var. V0634 CrA |Min II 13.9. V0648 CrA |Min II is felt at the phase 0.5P. V0659 CrA |P = 189.4d is possible. V0667 CrA |In the region of the bright cometary nebula NGC 6729. V0667 CrA |The spectral type is earlier than K. V0676 CrA |RR type is possible. V0686 CrA |Max I 5.34, Min I 5.41, Max II 5.35, Min II 5.40 [08970]. V0691 CrA |4U 1822-37. Emissions CIII/NIII lambda 4640 - 50, V0691 CrA |He II lambda 4686, CIV lambda 1550 etc. V0692 CrA |P = 0.83d is possible. eps CrA |Min II 4.95. R CrB |IR excess. S CrB |OH, H2O, SiO maser. T CrB |VB? A (B <= 12m, 0.2"). SB (P = 227.6d). T CrB |The spectral period is present in the photometric data of T CrB |1891 - 1917 and 1960 - 1971 [08978]. The epoch of the first T CrB |outburst JD2402734 (1866). Two smaller outbursts were T CrB |observed in UV light, JD2438030 (1963) and 2442543 T CrB |(1975) [08979]. U CrB |Min II 7.72. P var. RR CrB |P2 = 377d. Delta(m) (P1) ~0.5m, Delta(m) (P2) ~0.6m. RS CrB |P2 = 69.5d [01100]. Main period oscillation: 9.1m - 11.6m. RT CrB |Nonlinear term: +2.01d*10**(-8)*E**2. Min II 10.52 (var). RT CrB |DII = 0.09P. RV CrB |P var. Max = 2428285.608 + 0.3316217d*E (JD2428285 - 31610); RV CrB |Max = 2431705.349 + 0.3317313d*E RV CrB |(JD2431705 - 32954); Max = 2433030.572 + 0.331705d*E RV CrB |(JD2433030 - 36814) [05496]; Max = RV CrB |2440001.453 + 0.331569d*E (1967 - 1971) [06237]; RV CrB |Max = 2441451.413 + 0.331619d*E (1972 - 1974) RV CrB |[07032]. The Table gives current elements. On RV CrB |the period changes see also [03506]. Blazhko effect? RW CrB |d = 0.028P. Min II 10.29. TW CrB |Min II 11.0. TZ CrB |ADS 9979 A (B 6.72m, GIV, 6.6", 233deg, 1980). TZ CrB |SB2 (P = 1.139789d). TZ CrB |Epoch of Min is given. The variation presented in the TZ CrB |Table is superimposed by a second one, with the same TZ CrB |amplitude and P = 0.1d. The amplitude is given TZ CrB |for the combined light of ADS 9979 A and B, the TZ CrB |mean magnitude is for ADS 9979 A. UU CrB |During JD2444381.73 - .76 a slow flare was observed, with UU CrB |maximal amplitude 0.30m in the IK band and 0.18m in the UU CrB |U band. AL CrB |Spotted rotating G-type giant. alf CrB |lambda eff = 7230 A: DI = 0.034P, DII = 0.018P, alf CrB |Min II - Min I = 0.66P, depth of Min I 0.10m, Min II alf CrB |0.025m. bet CrB |VB A (B ~ 5m - 6m, 0.2", ~130deg, 1978). SB (P = 3833.7d). bet CrB |Magnetic field var, P = 18.487d. The epoch of Min light bet CrB |is given. gam CrB |ADS 9757 (4.2m, 5.6m; A = 0.74", P = 91.0a). U Crv |VB A (B 13.5m, 0.4' p). W Crv |Min II 11.86. The light curve is asymmetrical, the maxima W Crv |differ in hight by 0.10m. Y Crv |Min II 11.7. RRC type with twice shorter period Y Crv |is possible. Z Crv |d = 0.06P. RV Crv |Elements do RV Crv |not satisfy some of the published moments of Min. RZ Crv |Min II 13.9. SX Crv |Min II 9.23. The shape of the light curve varies. Depth of SX Crv |Min I 0.20m, depth of Min II 0.18m. In 1972 the system SX Crv |became fainter than in 1971 by 0.06m. TY Crv |SB2. R Crt |Periods of light constancy which last up to 250d occur R Crt |every two or there thousand days. OH, H2O maser. S Crt |H2O maser. T Crt |Mean light var, P2 = 1006d. V Crt |Min II 10.1; Min II - Min I = 0.57P. W Crt |(k - b)2 = +0.21. X Crt |(k - b)2 = +0.02. Z Crt |d = 0.016P. RR Crt |P = 293d or 146d is possible. RV Crt |Min II 9.4:. SU Crt |[Fe/H] > -0.3. SV Crt |ADS 8115 A (B 11.5m vis, 1", 220deg). SB2 (P = 5.90513d, SV Crt |apsidal motion, P ~700a). Epoch of Min I in B light is SV Crt |given. Depth of Min II is 0.015m. EuII and SrII in SV Crt |emission. R Cru |In the region of the open cluster NGC 4349. T Cru |In the region of the open cluster NGC 4349. U Cru |P var. Max = 2410143 + 351.4d*E (JD2410100 - 14100) [00237]; U Cru |since JD2437600 - see Table. W Cru |Min II 9.3. SU Cru |[A/H] = -0.8. SV Cru |In the region of the open cluster Ruprecht 97. SV Cru |Non-member of the cluster. SW Cru |VB A (B 14.0m, 12"). (k - b)2 = 0.27. SY Cru |d = 0.05P? TU Cru |Min II 11.5. TW Cru |Min II 12.85:. TX Cru |It is not excluded that actually P is much shorter, TX Cru |close to 1d, for instance. TZ Cru |P = 2.091140d? UW Cru |Min II 12.9; Min II - Min I = 0.536P. UX Cru |VB A (B 10"). Min II 12.4; Min I - Min II = 0.325P; UX Cru |DII = 0.025P. VY Cru |Min II 13.5. VZ Cru |P = 1.125810d? WW Cru |Min II 13.0. WX Cru |d = 0.040P. Light variability in maximum is noted. WY Cru |VB A. P = 9.013290d? XX Cru |P = 3.28566d? XY Cru |Min II 11.7. XZ Cru |P = 1.6495930d? YY Cru |Min II 13.0. YZ Cru |Min II 13.1. ZZ Cru |Min II 9.8. AB Cru |Min II 8.9. AC Cru |Min II 12.1. AD Cru |VB A (B 14.5m, 10", 270deg). P var. Max = 2434918.160 + AD Cru |6.39844d*E (JD2423800 - 35400) [02309]; AD Cru |since JD2441000 - see Table. AE Cru |Depth of Min II 0.03m. AF Cru |According to [01122] Algol-type with the elements: AF Cru |Min I = 2424988.959 + 1.895669d*E, D = 0.06P. AF Cru |This conclusion must be checked. The star deserves careful AF Cru |investigation. AG Cru |The blue component is possible [09004]. AI Cru |In the region AI Cru |of the open cluster NGC 4103. Min II 9.94. AQ Cru |Min II 13.8. AT Cru |Min II 12.6. AW Cru |Min II 13.9. AY Cru |Min II 11.2. BB Cru |Min II 14.0. BC Cru |Depth of Min II 0.03m. BD Cru |Depth of Min II 0.05m. BF Cru |Min II 12.3. BH Cru |Epoch of Min I is given in the Table. The light BH Cru |curve like the light curves of R Cen and R Nor BH Cru |has two maxima and two minima of different BH Cru |depths. Max I 7.6m (0.22P), Min II 8.0m (0.41P), BH Cru |Max II 7.2m (0.53P). BI Cru |Spectrum description [04949]. BK Cru |In Coalsack region. BM Cru |In Coalsack region. BP Cru |3U 1223-62. A unique X-system. Consists of an X-pulsar BP Cru |with pulse period 698s [09018] moving on an excentric BP Cru |orbit (E = 0.47) around the ellipsoidal B2 supergiant with BP Cru |orbital period of 41.51d. Accretion of the stellar wind BP Cru |from the primary star on the pulsar increases during the BP Cru |periastron passage. Therefore large X-flares are observed BP Cru |with the elements: T (X Max) = 2433158.09 + 41.51d*E. BP Cru |Optical flares are possible. BQ Cru |B - V: +1.13, +0.88. BS Cru |In the open cluster NGC 4755. BT Cru |In the open cluster NGC 4755. BU Cru |In the open cluster NGC 4755. BV Cru |In the open cluster NGC 4755. BW Cru |In the open cluster NGC 4755. DU Cru |The identification with NSV 06012 (SIMBAD) is wrong. bet Cru |VB A (B 11.4m, 44.3", 322deg; C 7.5m, 372", 23deg). bet Cru |Interferometric binary. Multiple periods (the total V bet Cru |amplitudes of corresponding oscillations are indicated bet Cru |in brackets): P0 = 0.2365072d (0.034m), P1 = 0.160466d bet Cru |(0.029m), P2 = 0.121383d (0.01m), P02 = 0.249373d bet Cru |(0.016m), P13 = 0.24273d (0.024m), P24 = 0.23931d bet Cru |(0.028m), P03 = 0.16342d (0.016m), P14 = 0.16171d bet Cru |(0.029m). tet 2 Cru |SB (P = 3.4380d). BCEPS, P > 1h? [08420]. lam Cru |Type ELL with lam Cru |P = 0.7902d is possible. Amplitude and shape of lam Cru |the light curve vary. The secondary oscillation lam Cru |(A = 0.007m) with the elements Max = 2441779.034 + lam Cru |0.1793d*E is possible. R Cyg |VB A (B 9.3m, 91", 14deg). S4/6e - S8/6e. T Cyg |VB A (B 10.03m, 10.2", 122deg; C 12m, 13.6", 197deg). U Cyg |VB A (B 7.8m, 63.5", 51deg). P var. Max = 2406455 + U Cyg |461.57d*E (JD2404590 - 13900); Max = 2414827 + U Cyg |470.76d*E (JD2413900 - 19940); Max = 2421806 + U Cyg |455.95d*E (JD2419940 - 27380); Max = 2427848 + U Cyg |472.85d*E (JD2427380 - 35750); since JD2435750 - see Table. W Cyg |There is a second oscillation with P = 235.3d. X Cyg |P var. Max = 2410190.86 + 16.3841d*E (JD2410100 - X Cyg |23370) [09028]; since JD2417000 - see Table. X Cyg |There is a square term in the elements given in the Table: X Cyg |+1.01d*10**(-7)*E**2. [A/H] = 0.4. Y Cyg |Min II 7.75; E = 0.1458. Apsidal motion: P = 47.6 yr. Y Cyg |There are sinusoidal terms in the elements: Y Cyg |+0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E)); Y Cyg |Min II = 2409454.9174 + 2.9963328d*E - Y Cyg |0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E)). Z Cyg |OH, H2O emission. RR Cyg |VB A (B 12.5m, 18.1", 58deg). RS Cyg |VB A (B 7.09m, 132", 355deg; C 9.3m, 56", 106deg). RS Cyg |Epoch of light minimum is given. The shape of the light RS Cyg |curve strongly varies. Double maxima are sometimes RS Cyg |observed (Min II at the phase 0.5P). RU Cyg |VB A (B 12.40m V, 10", 224deg; C 11.15m V, 19", 29deg). RV Cyg |VB A (B 10m, 142", 118deg). RY Cyg |In the region of the open cluster NGC 6883. RZ Cyg |The shape of the light curve strongly varies. Alternation RZ Cyg |of high and low maxima, as well as of shallow and RZ Cyg |deep minima is observed, as a rule: 9.8m <= Max <= 12.0m. RZ Cyg |11.8m <= Min <= 14.1m. SS Cyg |SB2 (P = 0.27512995d [08285]). SS Cyg |During maxima of brightness there are oscillations of SS Cyg |light and X-ray flux with amplitudes about 0.002m V SS Cyg |and periods changing between 7.29s and 10.90s [06102, SS Cyg |09032]. SU Cyg |P var. Max = 2421278.503 + 3.845507d*E (JD2414250 - SU Cyg |29000) [01559]; Max = 2433095.944 + 3.845664d*E SU Cyg |(JD2429000 - 33150) [00921]; since JD2434500 - see Table. SV Cyg |VB A (B 9.5m V, 145", 140deg). SW Cyg |Min II 9.30; d(V) = 0.018P; d(U) = 0.00P. P var. Min I = SW Cyg |2414782.448 + 4.572937d*E (JD2411340 - 16450); SW Cyg |Min I = 2418440.758 + 4.5727923d*E (JD2417060 - SW Cyg |19740) [00063]; Min I = 2421504.489 + 4.572729d*E SW Cyg |(JD2421470 - 24970); Min I = 2425185.550 + 4.5728386d*E SW Cyg |(JD2424960 - 29500); Min I = 2433160.669 + 4.5729841d*E SW Cyg |(JD2433000 - 36800) [09085]; Min I = 2438584.3081 + SW Cyg |4.57311736d*E (JD2438600 - 40560) [09085]; SW Cyg |since JD2441160 - see Table. SY Cyg |d = 0.040P. Possible depth SY Cyg |of Min II 0.03m. SY Cyg |P var. Min I = 2411659.568 + 6.00584d*E (JD2411600 - SY Cyg |17100); Min I = 2420001.571 + 6.005716d*E SY Cyg |(JD2418760 - 20760) [01961]; SY Cyg |Min I = 2437069.254 + 6.005626d*E SY Cyg |(JD2432800 - 37070) [05416]. SY Cyg |Mean elements given in the Table represent epochs of SY Cyg |Min I in the interval JD2414400 - 37070 up to +- 0.07d. SY Cyg |According to [04248] the apsidal motion with the period ~46 SY Cyg |years is possible. SZ Cyg |[A/H] = 0.5. P var [02392]. SZ Cyg |Mean elements given in the SZ Cyg |Table represent epochs of Max up to +- 0.5d. According SZ Cyg |to [09029] "the O - C diagram has a sinusoidal structure SZ Cyg |as is to be expected for a member of a binary system" SZ Cyg |with P orb = 65 years. TT Cyg |VB A (B 10.8m V, 70", 213deg; C 11.1m V, 83", 49deg; TT Cyg |D 10.7m V, 94", 268deg). TV Cyg |According to [03663] - spectrum G0. TX Cyg |[A/H] = -0.2. P var. Max = 2436793.138 + 14.708157d*E TX Cyg |(JD2415000 - 37000); since JD2436700 - see Table. UU Cyg |VB A (B 10.7m V, 3.6", 351deg). UV Cyg |VB A (B 10.8m V, 0.9", 79deg). UW Cyg |P var. Min I = 2419624.501 + 3.450797d*E (JD2410000 - UW Cyg |20750) [00526]; Min I = 2419624.501 + 3.450752d*E UW Cyg |(JD2419620 - 33000); Min I = 2433848.508 + 3.450740d*E UW Cyg |(JD2430000 - 41800); since JD2441800 - UW Cyg |see Table. Possible depth of Min II 0.05m. UX Cyg |P var. Max = 2432444 + 560.3d*E (JD2415670 - 32450); UX Cyg |Max = 2439352 + 578.0d*E (JD2432450 - 40500); UX Cyg |since JD2437600 - see Table. Sometimes rapid light UX Cyg |decreases on the ascending branch near Max are observed UX Cyg |[01563,01564]. H2O, OH, SiO maser. UY Cyg |Delta(S) = 3.8. UZ Cyg |VB A (B 10.8m, 28", 130deg). d = 0.032P; Min II 10.31. VV Cyg |Min II 13.2. P var? [03665]. VW Cyg |d = 0.035P; Min II 10.31. P var. Min I = 2417377.123 + VW Cyg |8.4305260d*E (JD2415660 - 17400); Min I = VW Cyg |2430444.061 + 8.4302826d*E (JD2417400 - 30450); VW Cyg |Min I = 2441116.868 + 8.4303917d*E + 4.31d*10**(-8)*E**2 VW Cyg |(JD2430450 - 41120) [07096]; since JD2440350 - see Table. VX Cyg |[A/H] = 0.2. P var. There is a square term in the VX Cyg |elemenmts +8.02d*10**(-7)*E**2. VZ Cyg |P var. Max = 2437103.945 + 4.8645598d*E(JD2416000 - VZ Cyg |41000); since JD2434000 - see Table. WW Cyg |d = 0.008P; Min II 10.16. P var [06144]. Mean elements: WW Cyg |Min I = 2416981.299 + 3.3176924d*E (JD2412000 - 31000) WW Cyg |[00063]; since JD2431000 - see Table. WZ Cyg |Min II 10.9. XX Cyg |[Fe/H] = -0.49. P var. Max = 2430671.1010 + XX Cyg |0.134865026*E(2416560 - 30000); since JD2430000 - see XX Cyg |Table. XZ Cyg |[Fe/H] = -1.2. P var. Max = 2417201.241 + 0.4665878*E - XZ Cyg |0.000107d*10**(-6)*E**2 (JD2414000 - 35000) [02550]; XZ Cyg |Max = 2438562.796 + 0.466570d*E (JD2434000 - 39800); XZ Cyg |Max = 2440445.789 + 0.466497d*E (JD2439800 - 41000) XZ Cyg |[06237]; Max = 2441453.3856 + 0.4664731d*E XZ Cyg |(JD2441000 - 42500) [07424]; Max = 2443028.641 + XZ Cyg |0.466438d*E (JD2442500 - 43800) [09101]; Max = XZ Cyg |2444142.650 + 0.466649d*E (JD2443800 - 44200) XZ Cyg |[09102]; since JD2444100 - see Table. XZ Cyg |Besides that the star has a strongly XZ Cyg |expressed Blazhko effect; the period of Blazhko effect XZ Cyg |varies, too [07424,07425]. 0.13P <= M - m <= 0.22P; XZ Cyg |0.90m <= A(B) <= 1.70m, 0.70m <= A(B) <= 1.30m; XZ Cyg |-0.05P < O - C < +0.05; XZ Cyg |Max A = 2417025.5 + 57.401d*E (JD2417000 - 38500); XZ Cyg |Max A = 2438881.7 + 58.387d*E (since JD2438500).[09103]. XZ Cyg |After JD2444000 XZ Cyg |Blazhko effect period probably decreased to 56.3d [09102]. ZZ Cyg |VB A (B 12.63m, 8.5", 43deg. ZZ Cyg |Total brightness variation range ZZ Cyg |is given. Min II 10.78. P var. Min I = 2417442.419 + ZZ Cyg |0.6286185d*E (JD2415000 - 25800) [07427]; ZZ Cyg |since JD2427950 - see Table. AA Cyg |S 6/3. AC Cyg |H2O maser. AD Cyg |S 5/5. AE Cyg |d = 0.039P; Depth of Min II 0.06m. AF Cyg |Light curve (1914 - 1956) [09104]. AF Cyg |Two more independent oscillations are superimposed: AF Cyg |P2 = 175.8d, P3 = 941.2d. AK Cyg |VB A (B 11.06m, A7, 20", 85deg). AV Cyg |P var. Max = 2420451.9 + 87.48d*E (JD2418782 - AV Cyg |24823); Max = 2427936.3 + 89.73d*E (JD2426326 - AV Cyg |28745); Max = 2429440.9 + 87.69d*E (JD2428820 - AV Cyg |31260); Max = 2436413.8 + 89.63d*E (JD2434610 - AV Cyg |37130); since JD2437450 - see Table. AV Cyg |0.27P <= M - m <= 0.50P. AX Cyg |VB A (B 10.2m, 18", 52deg). AY Cyg |In the region of the open cluster Dolidze 2. BB Cyg |P var. Max = 2426360 + 265.7d*E (JD2414900 - 26700); BB Cyg |Max = 2433091 + 258.6d*E (JD2426700 - 35500); Max = BB Cyg |2438354 + 266.9d*E (JD35500 - 40200) [09106]; BB Cyg |since JD2439200 - see Table. BF Cyg |P orb = 750d [05655]. BF Cyg |Irregular light variations and sometimes observed BF Cyg |brightenings by 2m - 3m are superimposed by semiregular BF Cyg |oscillations with the cycle 755d [01039,08044]. BG Cyg |P var. Max = 2421190 + 290.35d*E (JD2421150 - 29950); BG Cyg |Max = 2430546 + 307.3d*E (JD2429950 - 30850); Max = BG Cyg |2432872 + 289.5d*E (JD2430850 - 34920); BG Cyg |since JD2435100 - see Table. BI Cyg |VB A (B 9.4m, 126", 110deg). BO Cyg |D = 0.025P; Min II 12.0. BR Cyg |D = 0.020P; Min II 9.58. BS Cyg |SC 8/8. P var. Max = 2422655 + 420d*E (JD2422600 - BS Cyg |24750) [01161]; Max = 2425181 + 431.4d*E (JD2424750 - BS Cyg |26500) [01171]; since JD2437500 - see Table. BY Cyg |VB A (B 16m). BZ Cyg |[A/H] = 0.1. Double maximum. CD Cyg |[A/H] = 0.2. P var. CD Cyg |There is a square term in the elements: CD Cyg |+1.54d*10**(-6)*E**2. CG Cyg |VB A (B 11.8m, 1.3", 306deg; 1979.7). CG Cyg |10.10 <= Min II <= 10.44. P var. CG Cyg |Min I = 2422967.4248 + 0.63114347d*E CG Cyg |(JD2422900 - 38500); since JD2439000 - see Table. Combined CG Cyg |light range is given. Shape of the light curve varies CG Cyg |[08848]. CH Cyg |Semiregular light variations with the mean cycle 97d; CH Cyg |mean brightness varies with the cycle ~4700d [01169]. CH Cyg |There are also a cycle 725d [08849], rapid oscillations CH Cyg |(A <= 0.25m U) and flares [05350]. It is not excluded CH Cyg |that the system is an eclipsing one [06499]. CI Cyg |d = 0.084P. CI Cyg |Depth of eclipses ~0.8m. The eclipses of B star are CI Cyg |observed. Usually there are light fluctuations near mean CI Cyg |brightness ( ~12.1m). The outbursts last some dozens CI Cyg |and hundreds days. Light curves [06155,08044,08850, CI Cyg |08851]. Emissions of H, He I, He II, [O III], and N III. CM Cyg |S 4/6.5e. CU Cyg |P var. Max = 2422643 + 223.8d*E (JD2422600 - 26500); CU Cyg |since JD2426500 - see Table. CV Cyg |dI = 0.06P; Min II 11.33. P var. Min I = 2424458.348 + CV Cyg |0.9834523d*E (JD2414300 - 24500); since JD2424450 - see CV Cyg |Table. Shape of the light curve and Min I depth vary. CY Cyg |SC 2/7.5. CZ Cyg |P var. Max = 2424500 + 284d*E (JD2424500 - 33600) CZ Cyg |[03122]; since JD2432700 - see Table. DD Cyg |P var. Max = 2425465 + 148.30d*E (JD2424800 - 39000) DD Cyg |[01149]; since JD2439000 - see Table. DF Cyg |P var [01177,06107]. Mean DF Cyg |brightness varies: Min = 2411292 + 780.2d*E [01571]. DG Cyg |SiO maser? DH Cyg |OH emission? DK Cyg |dI = dII = 0.04P; Min II 10.90. P var. DK Cyg |Shape of the light curve and depth of Min II vary. DL Cyg |Min II 9.9. DM Cyg |P var. Max = 2425887.560 + 0.4198557d*E (JD2415200 - DM Cyg |25900) [03506]; Max = 2425887.5597 + 0.41985715d*E DM Cyg |(JD2425880 - 29250) [00522]; Max = 2433872.420 + DM Cyg |0.41985842d*E (JD2429250 - 37900) [03506]; Max = DM Cyg |2438677.708 + 0.4198619d*E (JD2438600 - 41250) DM Cyg |[07114]; since JD2441240 - see Table. DM Cyg |There is also Blazhko effect with the elements: DM Cyg |Max(O - C) = 2442978.97 + 26.01d*E [08853]; DM Cyg |-0.01 d< = O - C <= +0.01d. Delta(S) = 0. DQ Cyg |P = 180d? DT Cyg |P var. Max = 2424305.651 + 2.49913d*E (JD2424300 - DT Cyg |28500) [01183]; Max = 2432792.893 + 2.49934d*E DT Cyg |(JD2430000 - 36000); since JD2436000 - see Table. DV Cyg |P var. Max = 2425476 + 146.7d*E (JD2415200 - 29200); DV Cyg |since JD2432800 - see Table. DW Cyg |P var. Max = 2427603 + 279.6d*E (JD2416700 - 33500); DW Cyg |since JD2433500 - see Table. DX Cyg |Min II 14.2; Min II - Min I = 0.515P; DI = 0.22P, DX Cyg |DII = 0.12P. DY Cyg |Slow oscillations are superimposed by rapid ones with DY Cyg |A = 0.3m [03662]. According to [03148] type EB? DY Cyg |Min = 2436659.531 + 0.6990d(:)*E (JD2436600 - 37000) DY Cyg |[03148]. EE Cyg |Min II 14.5. EF Cyg |142d <= P <= 175d. EH Cyg |P var. Max = 2427608 + 276.90d*E (JD2416200 - 27610); EH Cyg |since JD2427800 - see Table. EI Cyg |Epoch of Max I is given; heights of Max I and Max II EI Cyg |differ strongly, the depths of Min I and Min II are almost EI Cyg |equal. Max I - Min I = 52d. EK Cyg |Observations are represented by the elements in the EK Cyg |interval JD2425200 - 37900 only. EM Cyg |Mean cycle varies in the range 19d - 33d [04248,09111]. EM Cyg |Depth of eclipses 0.25m V; elements of eclipsing system EM Cyg |light variations: Min = 2437882.8595 + 0.29090950d*E - EM Cyg |21d*10**(-12)*E**2 [08854]. EM Cyg |Sometimes there are light oscillations with periods EM Cyg |14.6s - 21.2s and an amplitude up to 0.4% [06102,09112]. EN Cyg |d = 0.012P. P var. Min = 2425181.311 + 2.2148998d*E EN Cyg |(JD2424880 - 29600) [00332]; since JD2433500 - see Table. ES Cyg |P var. Max = 2425146 + 157d*E (JD2425000 - 29300) ES Cyg |[00332]; since JD2432800 - see Table. EV Cyg |P var. Max = 2427740 + 259.1d*E (JD2425100 - 29100); EV Cyg |since JD2433500 - see Table. EV Cyg |The position of the star in the chart in [00530] is wrong EV Cyg |[00782]. EZ Cyg |P var? Shape of the light curve and the amplitude EZ Cyg |strongly vary; 0.40P < = M - m < = 0.48P. FF Cyg |S 5.5/6-e. FG Cyg |P var. Max = 2426955 + 456.0d*E (JD2416000 - 27000) FG Cyg |[00001]; Max = 2426955 + 458.8d*E (JD2426900 - 34300) FG Cyg |[03122]; since JD2439200 - see Table. FM Cyg |P var. Max = 2425313 + 274d*E (JD2425300 - 29200) FM Cyg |[00332]; since JD2429200 - see Table. FN Cyg |P var. Max = 2429137 + 314.6d*E (JD2416200 - 29200) FN Cyg |[00001]; since JD2432800 - see Table. FO Cyg |A var. P var. Max = 2425193 + 156.6d*E (JD2425000 - FO Cyg |29200) [00332]; since JD2432500 - see Table. FR Cyg |Min II 14.0; d = 0.03P. FT Cyg |P var. Max = 2425184 + 156.7d*E (JD2425100 - 29200) FT Cyg |[00332]. 83d <= P <= 187d (JD2432500 - 38000). FY Cyg |P var. Max = 2425172 + 194.d*E (JD2425100 - 29300) FY Cyg |[00332]. 130d <= P< = 189d (JD2432500 - 38000). GG Cyg |d = 0.079P; Min II 12.1. GM Cyg |P var. Min = 2428754.305 + 4.745772d*E (JD2413200 - GM Cyg |33500) [01209]; since JD2433500 - see Table. GN Cyg |P var. Max = 2425448 + 156d*E (JD2425400 - 27400) GN Cyg |[01155]; since JD2427500 - see Table. GO Cyg |Min II 8.73. P var. Intrinsic light variability of the GO Cyg |components is possible [01210]. GS Cyg |P = 195d? GT Cyg |Depth of Min II 0.05m? P var? GY Cyg |Secondary oscillation with P = 4000d and GY Cyg |A(V) = 0.5m is possible. GZ Cyg |Red. HL Cyg |d = 0.02P. HV Cyg |VB (Northern component). HY Cyg |P var. Max = 2425334 + 344d*E (JD2425300 - 29200) HY Cyg |[00332]; since JD2432760 - LB? II Cyg |P var. Max = 2425150 + 82d*E (JD2425120 - 25550), II Cyg |Max = 2425475 + 94d*E (JD2425550 - 29250) [00332]; II Cyg |since JD2432500 77d <= P <= 99d. IK Cyg |P var. Max = 2425199 + 77.3d*E (JD2425000 - 29200) IK Cyg |[00332]; since JD2432500 - see Table. IT Cyg |P var. Max = 2425305 + 67.4d*E (JD2425300 - 850) IT Cyg |[00332]; since JD2432500 - see Table. IU Cyg |B - V: +0.90, +1.45. P var. Max = 2429157.6 + 31.22266d*E IU Cyg |(JD2417800 - 29250); Max = 2433601.3 + 31.1550d*E IU Cyg |(JD2432700 - 35400); since JD2435400 - see Table. IV Cyg |P var. Max = 2425470.406 + 0.33432871d*E (JD2425300 - IV Cyg |33120) [03506]; Max = 2434122.519 + 0.33433895d*E IV Cyg |(JD2432700 - 40200) [04248]; since JD2440200 - see Table. IV Cyg |Shape of the light IV Cyg |curve varies: 0.10P <= M - m <= 0.20P. IX Cyg |P var. Max = 2425173 + 172d*E (JD2425000 - 25900) IX Cyg |[00332]; since JD2428000 - see Table. KL Cyg |P var. Max = 2437906 + 536.8d*E (JD2418500 - 38000) KL Cyg |[00001]; since JD2438000 - see Table. KP Cyg |Delta(S) = 0. KR Cyg |Min II 9.37. KU Cyg |Min II 11.15; d = 0.047P. Shape of the light curve varies. KV Cyg |Min II 11.9. KY Cyg |H2O, OH maser. LN Cyg |Min II 14.3. LO Cyg |Min II 13.3. LX Cyg |P var. Max = 2432775 + 460.0d*E (JD2415000 - 33300) LX Cyg |[01159]; since JD2437900 - see Table. SC 7/9-e - SC 8/8.5e. MQ Cyg |VB A (B 17.5m B, 4.5", 122deg). P var. Max = 2432737 + MQ Cyg |428.5d*E (JD2414300 - 33300) [01229]; since MQ Cyg |JD2440000 - see Table. MR Cyg |Min II 9.12; d = 0.030P; DII = 0.19P. MU Cyg |Min II 14.4. MY Cyg |Min II 8.99. Min II - Min I = 0.5021P. MZ Cyg |P var. Max = 2427641.914 + 21.162460d*E + MZ Cyg |0.10575d*10**(-3)*E**2 (JD2414900 - 37900) [03689]; since MZ Cyg |JD2443600 - see Table. Probably it is an RV Tau type MZ Cyg |variable, and then the period should be doubled [08862]. MZ Cyg |[A/H] = 0.1. NQ Cyg |EW type is possible. Close to V736 Cyg. NU Cyg |Min II 14.9. NZ Cyg |Min II 14.2. OS Cyg |P var. OU Cyg |Min II 15.6. OY Cyg |Star 23 - 30 [01321]. PP Cyg |Star G in the chart for VV245 [07749]. PR Cyg |Star 24 - 40 [01321]. PT Cyg |Star 23 - 55 [01321]. PU Cyg |Star 25 - 56 [01321]. PX Cyg |Star 35 - 78 [01321]. PY Cyg |Min II 15.2. QS Cyg |Min II 13.3. QT Cyg |Depth of Min II 0.04m. QU Cyg |Min II 15.1. QW Cyg |Min II 14.1. QX Cyg |Min II 14.5. V0339 Cyg |np component of a close binary. V0340 Cyg |Min II 14.5. V0343 Cyg |[A/H] = -0.2. V0346 Cyg |Companion 13.8m, 0.4' sf. Min II 11.9. P var. V0346 Cyg |Min I = 2427270.241 + 2.743345d*E (JD2415000 - 32000); V0346 Cyg |since JD2432000 - see Table. V0348 Cyg |According to [07516] EW type variable with large V0348 Cyg |irregularities: Min = 2441567.177 + 0.285768d*E V0348 Cyg |(JD2441567 - 95). V0355 Cyg |Min II 14.3. V0360 Cyg |P var [06107]. Min I = 2429187.4 + 70.449d*E V0360 Cyg |(JD2414600 - 34000) [00580]; since JD2426000 - see Table. V0366 Cyg |Min II 10.2. V0367 Cyg |VB A (A 0.1", 50deg; B 13.7m, 2.3", 255deg). Min II 7.16. V0367 Cyg |Shape of the light curve and the radial velocity curve V0367 Cyg |vary. V0368 Cyg |According to [00204] EB type (12.8m - 13.8m pg) V0368 Cyg |with the elements: Min I = 2425808.10 + 0.47586d*E V0368 Cyg |(JD2425805 - 853). V0369 Cyg |P var. Max = 2438199 + 104.46d*E (JD2426000 - 38200); V0369 Cyg |since JD2438200 - see Table. V0370 Cyg |Min II 11.9. P var. Min I = 2425096.429 + 0.77453979d*E V0370 Cyg |(JD2414400 - 30000); since JD2430000 - see Table. V0371 Cyg |Min II 12.5. V0374 Cyg |d = 0.03P. V0380 Cyg |Min II 5.76; Min II - Min I = 0.418P (1963). V0380 Cyg |There are periodic terms in the elements: V0380 Cyg |+0.8916d*sin(38.8deg + 0.0082deg*E) - V0380 Cyg |0.0796d*sin(77.6deg + 0.0164deg*E) + 0.0088d*cos(26.4deg + V0380 Cyg |0.0246deg*E); Min II = 2441262.266 + 12.425612d*E - V0380 Cyg |0.8916d*sin(38.8deg + 0.0082deg*E) - 0.0796d*sin(77.6deg + V0380 Cyg |0.164deg*E) - 0.0088d cos (26.4deg + 0.0246deg*E). V0380 Cyg |Apsidal motion is possible with P = 1490 years. V0382 Cyg |VB A (B 11.5m, 11", 332deg). Min II 9.12. V0382 Cyg |Shape of the light curve and depth of Min II vary. P var. V0382 Cyg |Min I = 2427992.458 + 1.885497d*E (JD2413480 - 29500) V0382 Cyg |[01253]; since JD2428000 - see Table. V0385 Cyg |Min II 12.4. V0387 Cyg |Min II 11.6. V0388 Cyg |Min II 9.15; d = 0.06P. P var. Min I = 2433584.540 + V0388 Cyg |0.8590507d*E (JD2427600 - 37200); V0388 Cyg |since JD2437200 - see Table. V0389 Cyg |VB A (B 8.0m, 3.4", 305deg, 1980). SB (P = 3.313168d); V0389 Cyg |Turns around the invisible third companion with V0389 Cyg |P = 154.09d. According to [01256] the light varies with V0389 Cyg |two alternate periods P1 and P2. The first oscillation V0389 Cyg |(P1) with A = 0.19m satisfies the elements: Max = V0389 Cyg |2423298.460 + 1.12912d*E, the second (P2) with A = V0389 Cyg |0.05m - the elements: Max = 2429162.080 + 1.19328d*E. V0389 Cyg |each of them continues for 1 - 3 weeks. At the transition V0389 Cyg |from one oscillation to the other irregular light V0389 Cyg |variations are sometimes observed or almost constant V0389 Cyg |brightness. At the renewal of each oscillation its phase V0389 Cyg |remains unchanged, experiencing no shift. According V0389 Cyg |to [08909] in 1975 - 1977 periodicity was not observed. V0393 Cyg |d = 0.02P. V0401 Cyg |Min II 11.13. P var. Min I = 2432881.277 + 0.582717d*E V0401 Cyg |(JD2428800 - 34000); since JD2434000 - see Table. V0402 Cyg |VB A (B 20", 90deg). V0407 Cyg |VB A (B 14.0m, 8", 190deg). V0407 Cyg |Light variations of the Mira type V0407 Cyg |variable are superimposed by the outburst of the probable V0407 Cyg |nova which occured near JD2428400 (1936) V0407 Cyg |with the consequent slow light decrease. Combined spectrum. V0411 Cyg |P var. Max = 2421075 + 321d*E (JD2421000 - 31100) V0411 Cyg |[01262]; since JD2431100 - see Table. V0416 Cyg |Red. V0425 Cyg |Description of the spectrum and its variations [02685,03149]. V0427 Cyg |P var. Max = 2425471 + 143d*E (JD2425400 - 5950) V0427 Cyg |[01155]; since JD2433850 - see Table. V0429 Cyg |In the region of the open cluster NGC 6883. V0430 Cyg |In the region of the open cluster NGC 6883. V0430 Cyg |Max = 2425544 + 258d*E (JD2425500 - 27400) [01155]. V0432 Cyg |In the region of the open cluster Dolidze 3. V0439 Cyg |In the region of the open cluster Berkeley 87 = OCL 161. V0441 Cyg |Epoch of Min I is given. V0442 Cyg |Min II 10.4:, d = 0.01P:. According to V0442 Cyg |[08721] the period given in [00525] must be doubled. V0443 Cyg |There is a periodic term in the elements: V0443 Cyg |-0.016d*sin(0.00105*E). V0444 Cyg |In the H II region S 109. Min II 8.06; V0444 Cyg |D II = 0.10P. P var. Min I = 2430856.453 + 4.21238d*E V0444 Cyg |(JD2415000 - 30000) [00007]; since JD2430000 - see Table. V0445 Cyg |P var. Min = 2425527.391 + 1.947833d*E (JD2425500 - V0445 Cyg |34700) [01155]; since JD2434700 - see Table. V0447 Cyg |In the region of the open cluster NGC 6871. V0448 Cyg |In the region of the open cluster NGC 6871. Min II 8.40. V0450 Cyg |The light curve resembles that of DQ Her. V0453 Cyg |In the region of the open cluster NGC 6871. Min II 8.68; V0453 Cyg |d = 0.03P; Min II - Min I = 0.5077P. [07518]. According to V0453 Cyg |[07518] there is apsidal motion with P = 71 years. V0454 Cyg |Min II 12.3. In the region of the open cluster IC 4996. V0455 Cyg |Min II 10.9. P var. Min I = 2431151.908 + 8.7689331d*E V0455 Cyg |(JD2426800 - 33950) [01286]; since JD2436800 - see Table. V0456 Cyg |Min II 11.4; Min II - Min I = 0.518P. P var? V0457 Cyg |Min II 13.9. V0458 Cyg |Min II 14.2. V0461 Cyg |PB ~7000d? [08251]. V0462 Cyg |P var. Max = 2428540 + 376.0d*E (JD2416000 - 35200); V0462 Cyg |since JD2435200 - see Table. V0463 Cyg |Min II 10.65; Min II - Min I = 0.514P. V0465 Cyg |There is a close companion of 17.5m. V0466 Cyg |Min II 11.4. V0469 Cyg |Min II 12.9; Min II - Min I = 0.57P. V0470 Cyg |Min II 8.545. V0471 Cyg |S 5.5/5.5. V0473 Cyg |P var. Max = 2430615 + 218.5d*E (JD2418000 - 31000) V0473 Cyg |[00346]; since JD2442300 - see Table. V0474 Cyg |d = 0.014P. V0477 Cyg |Min II 8.69; D II = 0.09P; d = 0.003P. P var. Min I = V0477 Cyg |2429194.309 + 2.3470011d*E (JD2410000 - 29200) V0477 Cyg |[00001]; Min I = 2437317.2695 + 2.3469943d*E V0477 Cyg |(JD2429200 - 39700) [08919]; since JD2439700 - see Table. V0477 Cyg |Apsidal motion with Pi = 349 years; E = 0.302 [06175]. V0477 Cyg |0.331P (1965 - 1970) <= Min II - Min I < = 0.460P (1904). V0478 Cyg |VB A (B 12.8m, 4", 259deg. Min II 9.02; Min II - Min I = V0478 Cyg |0.5072P. V0482 Cyg |VB A (B 14.4m V, M4 III, 8", 225deg). V0483 Cyg |Min II 11.9. V0484 Cyg |Min II 13.6. V0486 Cyg |Min II 14.3. V0488 Cyg |Min II 13.0. V0490 Cyg |Min II 13.5; Min II - Min I = 0.47P. V0491 Cyg |Min II 14.7. V0493 Cyg |Min II 12.9. V0494 Cyg |Min II 13.6. V0496 Cyg |Min II 12.5. V0498 Cyg |Min II 10.27. V0500 Cyg |VB B (A 11.5m; 18", 45deg). Min II 12.0. V0501 Cyg |Min II 13.1; d = 0.02P. V0502 Cyg |Min II 14.2. V0505 Cyg |Min II 12.0. V0509 Cyg |d = 0.05P. V0512 Cyg |Min II 11.5. There is a periodic term in the elements: V0512 Cyg |+0.065d*sin(0.2105263deg*(E + 538)). V0513 Cyg |Min II 12.6. V0519 Cyg |Min II 13.4. V0520 Cyg |VB A (B 15", 135deg). V0525 Cyg |d = 0.03P:. V0526 Cyg |Min II 13.1. In the region of the open cluster TGC 7039. V0532 Cyg |P var. Max = 2434618.158 + 3.283651d*E (JD2427900 - V0532 Cyg |35000); Max = 2436817.694 + 3.282792d*E (JD2435000 - V0532 Cyg |38700); since JD2438700 - see Table. V0536 Cyg |d = 0.010P. V0538 Cyg |B - V: +1.17, +1.50. V0539 Cyg |P2 = 1500d. V0541 Cyg |Min II 10.9; DII = 0.012P; Min II - Min I = 0.453P. V0544 Cyg |P var? V0546 Cyg |Min II 15.2:; Min II - Min I = 0.48P; d = 0.077P. V0546 Cyg |In the dark nebula Barnard 144. V0547 Cyg |B - V: +1.27, +1.73. In the dark nebula Barnard 144. V0548 Cyg |Min II 8.62. P var. Min I = 2442279.3838 + 1.80524695d*E V0548 Cyg |(JD2430800 - 42300) [08930]; since JD2442300 - see Table. V0563 Cyg |P var. Max = 2427590 + 295.4d*E (JD2426000 - 30250); V0563 Cyg |since JD2430250 - see Table. V0567 Cyg |d = 0.036P. V0581 Cyg |Red. V0586 Cyg |In the region of the open cluster NGC 7039. V0588 Cyg |VB A (B 18m, 15", 0deg). Very Red. V0589 Cyg |VB. V0606 Cyg |P var. Max = 2428376.7 + 50.245d*E (JD2427950 - 31330) V0606 Cyg |[01262]; since JD2437100 - see Table. V0612 Cyg |Cycles of 50 - 100d (JD2427950 - 31330) [01262]; V0612 Cyg |since JD2437100 - see Table. V0614 Cyg |Min II 14.5. V0618 Cyg |In the region of the open cluster TGC 7092. V0622 Cyg |In the region of the open cluster NGC 7092. V0628 Cyg |Min II 12.5. V0635 Cyg |Min II 13.5. V0643 Cyg |P var. Elements given in the V0643 Cyg |Table are valid in the interval JD2427950 - 31330. V0644 Cyg |VB A (B 15.6m, 6", 141deg; C 16.3m, 6", 141deg). V0645 Cyg |Observed as the V0645 Cyg |bright nebular condensation with ~2" diameter scattering V0645 Cyg |light of an O8 star associated with it but invisible V0645 Cyg |because of absorption. A part of strongly polarized V0645 Cyg |bipolar nebula with diameter about 10". There are V0645 Cyg |strong emission lines of H, Fe II, [O I], [S II], etc. In V0645 Cyg |the spectrum [08942,09129]. H2O maser source. Infrared V0645 Cyg |source CRL 2789. V0651 Cyg |Min II 14.7. V0652 Cyg |Min II 12.1. V0664 Cyg |d = 0.05P. V0666 Cyg |P var. Max = 2427965 + 236d*E (JD2427950 - 31350) V0666 Cyg |[01262]; since JD2433400 - see Table. V0670 Cyg |sp component of a close binary. V0680 Cyg |Min II 10.3. V0685 Cyg |VB. V0687 Cyg |Min II 10.4. P var? V0688 Cyg |d = 0.029P. V0690 Cyg |d = 0.021P. V0691 Cyg |d <= 0.034P. V0692 Cyg |Min II 14.9? V0693 Cyg |Min II 14.4? V0694 Cyg |d = 0.017P. V0695 Cyg |31 Cyg. Probably enters a common system with V1488 Cyg V0695 Cyg |(32 Cyg). VB A (B 13.0m, 36.8", 332deg; C 6.99m, 107.0", V0695 Cyg |174deg; D 5.0m, 338", 323deg). d = 0.0151P. V0695 Cyg |Interferometric binary eclipsing system (A = 0.08", V0695 Cyg |E = 0.15 [01582]; 0.035", 141.8deg, 1980.4). The epoch of V0695 Cyg |eclipse of the component of the spectral type B4 by the V0695 Cyg |component of the type K4 is given in the Table. The V0695 Cyg |amplitude strongly varies depending upon the wavelength: V0695 Cyg |A(lambda 6560 A) = 0.03m, A(lambda 3530 A) = 1.80m [09131]. V0696 Cyg |Mean magnitude varies with P = 1600d. V0700 Cyg |Min II 12.3. P var. Min I = 2432028.863 + 0.340047d*E V0700 Cyg |(JD2431700 - 37500) [05352]; since JD2437500 - see Table. V0704 Cyg |Min II 14.2. V0706 Cyg |Min II 13.9. V0713 Cyg |Min II 15.1. V0720 Cyg |P var. Min I = 2427611 + 332d*E (JD2429450 - 32000) V0720 Cyg |[00798]; since JD2432500 - see Table. V0726 Cyg |Min II 12.8; d = 0.018P. V0728 Cyg |P var. Min = 2425760.475 + 2.0601256d*E (JD2425500 - 35000) V0728 Cyg |[00164]; since JD2439700 - see Table. V0729 Cyg |VB A (B 13.5m, 1.5", 65deg). Min II 9.29. P var. Min I = V0729 Cyg |2434264.638 + 6.597700d*E (JD2428700 - 37900) V0729 Cyg |[00001]; since JD2439750 - see Table. V0731 Cyg |VB. V0735 Cyg |Depth of Min II 0.04m. V0736 Cyg |Min II 16.5. Close to NQ Cyg. V0737 Cyg |Star 23 - 50 [01321]. V0739 Cyg |Star 36 - 81 [01321]. V0741 Cyg |d = 0.03P. V0742 Cyg |P var. Max = 2429409.448 + 0.93979d*E (JD2428420 - V0742 Cyg |30700) [08977]; Max = 2431489.580 + 0.94010d*E V0742 Cyg |(JD2430250 - 32350); Max = 2433282.014 + 0.93979d*E V0742 Cyg |(JD2432350 - 33650); since JD2433650 - see Table. V0742 Cyg |According to [08977] since JD2430700 the observations are V0742 Cyg |better represented by the elements: V0742 Cyg |Max = 2432943.701 + 0.93977897d*E - 1.067d*10**(-7)*E**2. V0747 Cyg |The intervals between maxima of brightness V0747 Cyg |are 2000 - 4000d. Not red. V0751 Cyg |In the region of the nebula IC 5070. SB (P = 0.25d [09132]). V0751 Cyg |Rapid small variations near maximum of brightness V0751 Cyg |(<B - V> = +0.25) are superimposed sometimes by deep V0751 Cyg |minima lasting for some hundreds days [02699]. Soft X-ray V0751 Cyg |source [09133]. Spectrum description [02698,09132]. V0752 Cyg |<B - V> = +0.77, <U - B> = -0.47. V0753 Cyg |d = 0.12P. P = 0.952374d? V0757 Cyg |Red. V0758 Cyg |P = 400d? V0759 Cyg |P var. Max = 2434513.427 + 0.36001476d*E V0759 Cyg |(JD2414430 - 34570) [03506]; since JD2434500 - see Table. V0759 Cyg |Blazhko effect. V0779 Cyg |Type RR? V0781 Cyg |P var? V0783 Cyg |P var. Max = 2433261.029 + 0.62069487d*E V0783 Cyg |(JD2424690 - 34000); since JD2438970 - see Table. V0786 Cyg |Usually in minimum brightness, with rapid V0786 Cyg |brightenings by 0.5m - 1.0m. In the interval JD2427692 - V0786 Cyg |697 the brightness was 13.5m. V0789 Cyg |P var? [Fe/H] = -0.91. V0795 Cyg |sf component of a close pair. V0796 Cyg |Min II 11.4. V0797 Cyg |Min 15.4. V0799 Cyg |P var. V0801 Cyg |There is a square term in the elements: V0801 Cyg |+1.93d*10**(-10)*E**2. V0802 Cyg |P var. Max = 2432779.9342 + 0.59560377d*E V0802 Cyg |(JD2425480 - 35170) [02775]; Max = 2439415.263 + V0802 Cyg |0.5955638d*E (JD2435950 - 40000) [09266]. Max = V0802 Cyg |2440036.409 + 0.595447d*E (JD2440000 - 41000); Max = V0802 Cyg |2441517.498 + 0.595635d*E (JD2441000 - 42500); V0802 Cyg |since JD2442500 - see Table. Shape of the light curve V0802 Cyg |varies (0.13P <= M - m <= 0.50P); period variations are V0802 Cyg |accompanied sometimes by strong variations of amplitude V0802 Cyg |(in the interval JD2440000 - 41000; 0.3m <= A <= 1.7m). V0803 Cyg |Min II 14.5. V0806 Cyg |Min II 15.0; DII = 0.061P. V0807 Cyg |Min II 14.9. V0808 Cyg |Brightness in maximum varies. V0809 Cyg |Min II 13.6; DII = 0.069P. V0810 Cyg |d = 0.050P. Depth of Min II 0.05m. P var? V0817 Cyg |sp component of the pair. V0818 Cyg |Shape of the light curve and period vary. V0821 Cyg |Min II 15.6. V0822 Cyg |Min II 13.0. V0824 Cyg |Min II 14.3. V0825 Cyg |Min II 16.9. Min II = 2433871.915 + 7.709015d*E. V0826 Cyg |Min II 14.7. V0828 Cyg |Min II 10.12. V0832 Cyg |VB A (B 9.43m, 20", 352deg; C 11.62m, 27", 141deg; D 12.72m, V0832 Cyg |38", 220deg). description of spectral variations [09135]. V0836 Cyg |Min II 8.77. P var. Min I = 2426547.5224 + 0.65341090d*E V0836 Cyg |(JD2425500 - 42000) [03869]; since JD2441200 - see Table. V0836 Cyg |Shape of the light curve varies. V0840 Cyg |LS II 28.3deg [08090]. Cycles 250 - 300d. V0841 Cyg |Min II 11.2. V0842 Cyg |Min II 14.1. V0844 Cyg |VB A (B 17.8m, 2.9", 50deg). V0850 Cyg |Min II 11.8. P var. Min I = 2430587.263 + 4.5578d*E V0850 Cyg |(JD2428750 - 30590) [04253]; since JD2434330 - see Table. V0851 Cyg |d = 0.017P? V0852 Cyg |Min II 14.9. V0853 Cyg |Min II 14.2. V0856 Cyg |Depth of Min II 0.05m. V0857 Cyg |Depth of Min II 0.03m. V0859 Cyg |Min II 12.1. V0865 Cyg |Min II 14.6. V0866 Cyg |Min II 13.9. V0869 Cyg |Min II 14.8. Shape of the light curve varies. V0870 Cyg |Min II 15.8. V0871 Cyg |Min II 14.9. V0873 Cyg |Min II 14.7. Min II - Min I = 0.48P. V0874 Cyg |Min II 13.8. V0877 Cyg |Min II 12.9. V0880 Cyg |Min II 14.1; Min II - Min I = 0.506P; d = 0.02P. V0881 Cyg |Delta(S) is small [09037]. V0882 Cyg |[Fe/H] = -1.42. V0884 Cyg |np component of a pair. Min II 14.2. V0885 Cyg |Min II 10.2. V0886 Cyg |Min II 14.1; Min II - Min I = 0.515P. V0887 Cyg |Depth of Min II 0.03m. V0888 Cyg |Min II 15.9. V0889 Cyg |Min II 10.4. V0891 Cyg |Min II 9.4. V0892 Cyg |Min II 15.5. nf component of a close pair. V0900 Cyg |Min II 15.2. V0902 Cyg |d = 0.02P. Depth of Min II 0.05m. V0906 Cyg |Min II 15.7. V0907 Cyg |Min II 14.9. According to [04427] Min I = V0907 Cyg |2435066.257 + 0.54138554d*E. V0908 Cyg |nf component of a close pair. Depth of Min II 0.04m. V0909 Cyg |Min II 9.66. V0910 Cyg |Min II 14.2; d = 0.02P. V0911 Cyg |Min II 14.6. P var? Min I = 2432120.251 + 3.42262215d*E V0911 Cyg |(JD2415500 - 37900) [04761]; since JD2437100 - see Table. V0912 Cyg |Depth of Min II 0.05m. V0913 Cyg |VB A (B 17m, 0deg). V0920 Cyg |A var. Blazhko effect? V0922 Cyg |d = 0.02P:. V0924 Cyg |P var. Max = 2435706.776 + 5.5709816d*E (JD2432760 - 38000) V0924 Cyg |[08053]; since JD2438000 - see Table. V0925 Cyg |Min II 16.0. V0927 Cyg |Epoch of Min brightness is given. V0928 Cyg |Min II 15.4. V0931 Cyg |Min II 14.5. V0932 Cyg |Depth of Min II 0.04m. V0934 Cyg |Min II 13.7. V0936 Cyg |Depth of Min II 0.05m. V0939 Cyg |Min II 12.5. V0940 Cyg |Min II 15.1. V0941 Cyg |Min II 13.2. V0942 Cyg |VB A (B ~10deg, C ~110deg). V0944 Cyg |np component of pair. V0947 Cyg |Min II 15.0. V0948 Cyg |Min II 15.2. V0949 Cyg |Red. V0955 Cyg |Min II 15.3. sp component of a close pair. V0956 Cyg |Min II 15.1. sp component of a close pair. V0957 Cyg |Min II 12.6. V0958 Cyg |P = 199d? V0959 Cyg |Min II 11.4; Min II - Min I = 0.52P; DII = 0.16P:. V0959 Cyg |sp component of a close pair. V0961 Cyg |Min II 12.4; Min II - Min I = 0.505P. V0962 Cyg |d = 0.02P:. V0964 Cyg |Min II 14.4. V0965 Cyg |Min II 14.9. Type RRC? P = 0.32028628d? V0970 Cyg |Min II 14.8. V0974 Cyg |Min II 12.5; Min II - Min I = 0.462P. V0974 Cyg |Min II = 2435373.398 + 3.204418d*E. V0979 Cyg |Min II 14.7. V0981 Cyg |Min II 15.0. V0982 Cyg |Red. V0997 Cyg |[Fe/H] = -0.77. V1004 Cyg |Min II 13.0. V1007 Cyg |Depth of Min II 0.04m. V1008 Cyg |Min II 16.0. V1010 Cyg |Depth of Min II 0.03m. V1011 Cyg |Depth of Min II 0.04m. V1012 Cyg |Min II 15.4. V1016 Cyg |Before the outburst in 1964 the brightness V1016 Cyg |changed between 15.0m and 17.5m pg [05701], the spectral V1016 Cyg |type was late Me alpha [01222]. In the 1964 - 67 the V1016 Cyg |brightness increased from 16.0m to 11.2m B. In 1967 - 69 V1016 Cyg |the brightness steadily increased to 10.05m B, V1016 Cyg |being constant in V system (10.5m). In the infrared it V1016 Cyg |changes in the limits 6.9 - 8.4 J, 4.7 - 5.8 K with the V1016 Cyg |period 470d [07174,09141]. High excitation emission V1016 Cyg |spectrum with strong IR excess resembles that of V1016 Cyg |symbiotic variables [09142]. X-ray and radio source. V1018 Cyg |Min II 11.6. V1021 Cyg |Min II 14.3. V1023 Cyg |Min II 12.9; d = 0.03P:. DII = 0.14P. V1023 Cyg |Min II - Min I = 0.495P. V1024 Cyg |Depth of Min II 0.04m. V1030 Cyg |Elements given in the V1030 Cyg |Table are valid in the interval JD2426600 - 32300. V1033 Cyg |P var. V1034 Cyg |Min II 9.9. V1035 Cyg |P var? V1037 Cyg |Min II 14.8. V1038 Cyg |VB B (9.4", 215deg, 1963). Min II 15.5. V1039 Cyg |Min II 15.6. V1042 Cyg |VB A (B 10m, 53", 110deg). In HII region S 109. V1044 Cyg |Min II 16.5. V1045 Cyg |Min II 16.0. V1047 Cyg |d = 0.02P. V1053 Cyg |d = 0.05P. V1057 Cyg |In the dark nebula, in the region of the North America V1057 Cyg |nebula (NGC 7000). In 1969 - 70 (JD2440400 - 830) V1057 Cyg |the outburst from 16.5m to 10.3m occured. Brightness V1057 Cyg |maximum was observed at JD2440830 (spectrum - B3). V1057 Cyg |Before the outburst the light changed in the range V1057 Cyg |15.5m - 16.5m, the spectral type was Ke with V1057 Cyg |characteristic features of T Tau type stars [02698,06415]. V1057 Cyg |After the outburst the brightness began to weaken V1057 Cyg |monotonouosly and in 1982 reached 13.1m B (the spectral V1057 Cyg |type about G2 - G5 Ib). Strong Halpha emission appeared V1057 Cyg |in 1971. There are also small rapid light fluctuations. V1057 Cyg |Description of light variations [06504,07115, V1057 Cyg |07754, 08996]. The star is associated with a luminous V1057 Cyg |arc-shaped reflection nebula. This nebula with length V1057 Cyg |of about 3' appeared in 1971 and its brightness is V1057 Cyg |gradually decreasing simultaneously with the fading V1057 Cyg |of the star. V1061 Cyg |Min II 9.5. V1063 Cyg |P var. Max = 2428260 + 339d*E (JD2428260 - 30700); V1063 Cyg |since JD2433500 - see Table. V1064 Cyg |Min II 15.3. V1068 Cyg |Min II 11.2; d = 0.070P. V1068 Cyg |A migrating wavelike distorsion with an amplitude ~0.1m V V1068 Cyg |is being observed outside eclipses [08999]. V1073 Cyg |Min II 8.57. V1074 Cyg |Min II 14.8. V1083 Cyg |Min II 11.2. V1085 Cyg |Observations given in [07010] contradict the elements given V1085 Cyg |in [07193]: Min = 2437856.592 + 2.8089d*E. V1096 Cyg |d = 0.03P. V1102 Cyg |Radio-quiet N galaxy. Absorption spectrum without emission V1102 Cyg |lines; z = 0.0272. V1111 Cyg |Blazhko effect is possible. V1122 Cyg |Blazhko effect is possible. V1130 Cyg |Min II 12.9. V1136 Cyg |Min II 13.2. Eccentric orbit (E = 0.3). Apsidal motion is V1136 Cyg |possible [08051]. V1141 Cyg |Min II 11.8. V1142 Cyg |Min II 13.4. V1143 Cyg |Min II 6.06; Min II - Min I = 0.743P; d = 0.002P. V1157 Cyg |Min II 13.6. V1158 Cyg |d = 0.02P; Depth of Min II 0.04m. V1161 Cyg |d = 0.01P. V1162 Cyg |Only one Max was observed (see Table). Thereafter - either V1162 Cyg |invisible, or fairly constant (17.6m - 17.8m). Bluish. V1171 Cyg |VB A (B 11.0m, 0.34", 71.2deg; 1979.5). Min II 10.3. V1175 Cyg |Min II 16.5. P var. Min I = 2434629.545 + 1.3330d*E V1175 Cyg |(JD2426620 - 34630); since JD2434635 - see Table. V1176 Cyg |VB. Variable is probably the northern red component. V1187 Cyg |In the nebula IC 1318B. Min II 11.19. P = 3.7675d? V1188 Cyg |Min II 14.3. V1189 Cyg |Min II 13.7. P var. Min I = 2437906.516 + 1.041908d*E V1189 Cyg |(JD2426620 - 31240); since JD2437906 - see Table. V1191 Cyg |In the nebula IC 1318B. VB A (B 13m, 11", 299deg; C 13m, V1191 Cyg |11", 284deg). Min II 11.11. Shape of the light curve varies. V1193 Cyg |Min II 14.3. V1196 Cyg |Depth of Min II 0.05m. V1200 Cyg |Min II 16.1:. V1210 Cyg |Red. V1212 Cyg |Red. V1218 Cyg |VB A (B 17m, sf). V1225 Cyg |VB A (B 16m V, B - V = +1.3m, 1.2", 270deg; C 15.0m V, V1225 Cyg |B - V = +0.5m, 2.4", 270deg); P var? Max = 2428250 + V1225 Cyg |384.2d*E (JD2428200 - 38250) [03160]; since V1225 Cyg |JD2438500 - see Table. V1236 Cyg |Red. V1255 Cyg |Brightness in Max varies in the range 15.2m - 16.0m with V1255 Cyg |possible elements: Max = 2439382.281 + 0.28619537d*E. V1256 Cyg |Min II 14.1. V1273 Cyg |Min II 16.5. V1275 Cyg |In the region of the open cluster NGC 6819. V1281 Cyg |Min II 15.4. V1285 Cyg |Red. V1302 Cyg |Depth of Min II 0.05m. V1305 Cyg |Min II 11.5m - 11.7m (var). V1307 Cyg |Considerable dispersion of mean light curve points. V1315 Cyg |Min II 15.3. V1316 Cyg |(P) > 100d. V1318 Cyg |LkH alpha 225. Associated with a cometary nebula. V1321 Cyg |P = 0.7281802d? V1322 Cyg |In the region of the open cluster NGC 6913. V1326 Cyg |Min II 11.8; Min II - Min I = 0.53P. V1327 Cyg |Very red. V1329 Cyg |In 1891 - 1964 light variations in the range 14.2m - 15.5m V1329 Cyg |with deep minima to 18m; the minima are satisfied by the V1329 Cyg |elements given in the Table; D = 0.1p; spectral type M V1329 Cyg |[07235]. In 1964 - the outburst up to 12.1m. Then gradual V1329 Cyg |brightness decrease superimposed by periodical V1329 Cyg |variations with an amplitude near 1m. Light minima V1329 Cyg |as before are satisfied by the elements given in the V1329 Cyg |Table but the character of eclipses changed (probably V1329 Cyg |because of appearance of a dense envelope ejected V1329 Cyg |by one of the components of the system). After the V1329 Cyg |outburst high excitation emission spectrum with IR V1329 Cyg |excess is observed similar to the spectrum of symbiotic V1329 Cyg |variables. V1331 Cyg |Associated with a cometary nebula. V1334 Cyg |VB A (B 7.9m, B5 - B8, 0.13", 26.1deg, 1975). V1336 Cyg |According to [07010], RR? P = 0.5d? V1341 Cyg |Cyg X-2. SB1. Halo object (nu = -220 km/s). Strong V1341 Cyg |reflection effect changes the spectral type of the F V1341 Cyg |component. Spectral line profiles vary. The lines of V1341 Cyg |He II, KCa II, C III,and N III are in emission. The V1341 Cyg |system has low and high states. During the low state the V1341 Cyg |mean light curve is a double wave with the range V1341 Cyg |15.1m - 15.4m B. Epoch of Min I given in the Table V1341 Cyg |corresponds to the F star in superior conjunction; V1341 Cyg |Min II 15.4. The eclipse of the accretion disk at the V1341 Cyg |phase 0.5P in partial. Rapid light variability by 0.1m V1341 Cyg |in 10 minutes and by 0.5m in several hours is V1341 Cyg |superimposed. In the high states lasting V1341 Cyg |for ~10d the mean light increases by 0.5m. Radio V1341 Cyg |source at 8085 MHz, source of soft and hard X-ray V1341 Cyg |emission from 0.1 to 60 KeV. V1345 Cyg |Min II 15.0:. V1354 Cyg |Depth of Min II 0.04m. V1356 Cyg |Min II 10.4. V1357 Cyg |Cyg X-1. SB1. The epoch of the inferior conjunction of the V1357 Cyg |optical component is given in the Table. Min II 8.88. The V1357 Cyg |shape of the light curve varies; Min II sometimes are not V1357 Cyg |observed. The periodicity in the light curve variations V1357 Cyg |as well as in polarization changes is possible with V1357 Cyg |P = 78.4d [09021,09022]. Rapidly variable X-ray source in V1357 Cyg |wide range up to 3 MeV characterized by the change of high V1357 Cyg |and low states. Light and X-ray variation with P = 294d V1357 Cyg |is also detected [09154,09156]. Variable and flare radio V1357 Cyg |source at 2695 and 8085 MHz. V1372 Cyg |P2 = 360d?. V1374 Cyg |Min II 17.7. V1384 Cyg |In the region of the open cluster NGC 6913. V1396 Cyg |VB AB (10.26m V, 12.3m V; A = 0.1127", P = 29.33 Y V1396 Cyg |[09026]); mu = 0.67", P = 113deg; A-SB 2 (mAb - mAa = 0.6m, V1396 Cyg |P = 3.275631d [09025]). Probably all the three components V1396 Cyg |of the system are variables of the UV Cet type, and V1396 Cyg |according to [05716] also of the BY Dra type. The range of V1396 Cyg |combined brightness of the system is given in the Table. V1396 Cyg |Really the flare of AB component was observed in the V1396 Cyg |spectrograms [09025]. V1401 Cyg |Min II 13.6. V1410 Cyg |P > 400d. V1411 Cyg |P = 1.553478d? V1412 Cyg |Min II 15.5. V1414 Cyg |Northern component of a close pair; d = 0.04P. V1416 Cyg |Min II 14.7. V1417 Cyg |Min II 13.1. V1421 Cyg |In the region of the planetary nebula NGC 6857 = K3 - 50. V1425 Cyg |Depth of Min II 0.31m. V1427 Cyg |In the region of the open cluster M39. V1429 Cyg |Min II 15.3. V1430 Cyg |Min II 15.0. V1436 Cyg |Min II 15.9, D II = 0.08P; Min II - Min I = 0.48P. V1437 Cyg |Min II 16.0. V1440 Cyg |In the region of the open cluster NGC 6819. V1465 Cyg |Resembles an eclipsing variable. V1478 Cyg |VB A (B 17m:, 3", 80deg). V1478 Cyg |Compact radio source. extended structure centered at the V1478 Cyg |star is observed at 5 Ghz. Bq [] star with the excess of V1478 Cyg |infrared radiation of dust at T = 300degK. Description of V1478 Cyg |the spectrum [07080,07081,07523,09159,09160]. V1479 Cyg |In the region of the nebula IC 5070. V1481 Cyg |Min II 12.5. In the region of the open cluster NGC 7128. V1485 Cyg |Identical to VES 28, as it follows from latter star's V1485 Cyg |coordinates and magnitudes in [7095], but the star is V1485 Cyg |actually invisible in the chart in [7095], where a faint V1485 Cyg |companion, to 0.4'N of the variable, is erroneously marked. V1485 Cyg |Similarly, it is identical to +29deg 104, judging from the V1485 Cyg |latter star's photometry and spectral type from [4732]; V1485 Cyg |however, the star is plotted slightly offset (by 0.8' to E) V1485 Cyg |in the chart in [4732]. V1488 Cyg |32 Cyg. Probably enters a common system with V695 Cyg V1488 Cyg |(31 Cyg). 0 < d < 0.011P. P var. V1488 Cyg |Min I = 2420670.0 + 1140.1d*E (JD2411400 - 29700). V1488 Cyg |Since JD2429700 - see Table. V1488 Cyg |The epoch of the eclipse of the B4 type V1488 Cyg |Component by the K5 type component is given. There V1488 Cyg |is also small physical light variability of the K V1488 Cyg |component [08896,09161]. Depth of eclipses depends of lambda: V1488 Cyg |0.04M V, 0.13m B, 0.27m (lambda 4243A),0.90m (lambda 3552A). V1489 Cyg |NML Cyg. 17.0m: - 18.0m V, B>21M; I - K = +8.17. V1489 Cyg |Very large IR exess due to expanding gaseous-dust envelope. V1489 Cyg |In the area 2.5"*3.5" around V1489 Cyg |the star the system of about 60 discrete sources of V1489 Cyg |OH emission is detected [07461]; source of OH, H2O, V1489 Cyg |SiO maser emission. Light variations are periodical V1489 Cyg |(see also [09163]). The object may be a protostar being V1489 Cyg |observed at the end of condensation process. The late V1489 Cyg |spectrum arises probably in the extending envelope V1489 Cyg |[09165,09166]. V1490 Cyg |In the region of the nebula IC 5070. V1491 Cyg |In the region of the nebula IC 5070. V1492 Cyg |In the region of the nebula IC 5070. V1493 Cyg |In the region of the nebula IC 5070. V1707 Cyg 10.5"P. V1494 Cyg |In the region of the nebula IC 5070. V1495 Cyg |In the region of the nebula NGC 7000. V1497 Cyg |In the region of the nebula NGC 7000. V1498 Cyg |In the region of the nebula NGC 7000. V1500 Cyg |In August 1975, before the very rapid increase V1500 Cyg |of light, the brightness of the Nova gradually increased V1500 Cyg |from 17.6m to 13.5m B (JD2442632 - 653.2). After Max V1500 Cyg |almost monotonous decay of brightness is superimposed by V1500 Cyg |light variations with the amplitude of 0.03m - 1.0m V; V1500 Cyg |the period of these variations in the interval V1500 Cyg |JD2442656 - 43100 changed in the range 0.1415d [09167, V1500 Cyg |09168] - 0.137d [09169,09170]. Since JD2443100 Min = V1500 Cyg |2443696.4827 + 0.1396133d*E. Some investigators (see, V1500 Cyg |for instance, [09173]) adopt double value of this peiod. V1500 Cyg |A month after the light maximum of the Nova the V1500 Cyg |radio emission was registered at 2695 and 8085 MHz [09171]. V1507 Cyg |The epoch of a broad Min I (superior conjunction of V1507 Cyg |the B component) is given; Min II 7.01; D II = 0.20P, V1507 Cyg |Min II - Min I = 0.29P; e = 0.39. Unusual light curve V1507 Cyg |[08213,09049]. Shape of the light curve and depths of V1507 Cyg |Min vary. Gaseous streams And expAnding envelope. V1508 Cyg |Min II 13.3. V1509 Cyg |VB A (B 11.7m, 55", 106deg). V1511 Cyg |V - K = 13.6m. V1513 Cyg |Gliese 781; mu alpha = -0.146S, mu delta = -1.00"; SB. V1515 Cyg |In a dark nebula, near the nebula NGC 6914. Connected V1515 Cyg |with nebular appendage like a Comma. Light increase was V1515 Cyg |observed from 1944 till 1958. Since 1958 the star is in V1515 Cyg |Max. Slow light variations with A <= 1.6m. The absorption V1515 Cyg |line Li I lambda 6707A is seen in the spectrum. V1521 Cyg |Cyg X-3. Peculiar infrared X-ray source. V > 23m. V1521 Cyg |Flare radio source. In the K band short and slow flares V1521 Cyg |on the time scale about 2 minutes and 1-2 hours, V1521 Cyg |irregular variations and longperiodic variability are V1521 Cyg |observed [07752]. These variations are accompanied V1521 Cyg |by periodical oscillations of infrared, X-ray and gamma V1521 Cyg |radiation with the elements: Min = 2440949.8986 + V1521 Cyg |0.1996830d*E + 1.25d*10**(-10)*E**2 [09187]. Usually the V1521 Cyg |amplitude of these variations A(K) = 0.5m, but sometimes V1521 Cyg |they disappear completely. V1523 Cyg |Amplitude and mean brightness strongly vary. V1531 Cyg |LkH alpha 142. VB A (B = V1532 Cyg, 2.5", 90deg). In the V1531 Cyg |region of the nebula IC 5070. Combined brightness and V1531 Cyg |spectrum are given. V1532 Cyg |LkH alpha 143. VB B (A = V1531 Cyg; B 2.5", 90deg). V1532 Cyg |In the region of the nebula IC 5070. Combined brightness V1532 Cyg |and spectrum are given. V1535 Cyg |In the region of the nebula IC 5070. V1536 Cyg |In the region of the nebula NGC 7000. V1538 Cyg |In the region of the nebula NGC 7000. V1539 Cyg |In the region of the nebula NGC 7000. V1540 Cyg |In the region of the nebula NGC 7000. V1546 Cyg |In the region of the nebula NGC 7000. V1548 Cyg |VB A (B 16.7m, 6.2", 131deg). V1554 Cyg |VB A (B 14.7m, 3.5", 214deg). V1577 Cyg |In the cluster and nebula IC 5146. V1578 Cyg |In the cluster and nebula IC 5146. VB A (B 15m, 5", 45deg; V1578 Cyg |C 17m, 5", 225deg). Associated with a reflecting nebula. V1580 Cyg |There is a periodic term in the elements: V1580 Cyg |-0.027d*sin(0.045deg) (JD - 2439000). V1581 Cyg |G 208 - 44. VB A (B = G 208 - 45, 15.97m V, M6Ve; 7.9", V1581 Cyg |106deg, 1954; 8.2", 96deg, 1974). mu = 0.71", P = 140deg. V1581 Cyg |The flare was observed during spectroscopic observations V1581 Cyg |[09175]. The companion may be also a UV Cet type variable. V1581 Cyg |The range of combined brightness variation of the system V1581 Cyg |is given. V1584 Cyg |Epoch of min brightness is given. V1597 Cyg |In the region of the nebula IC 5070. V1598 Cyg |In the region of the nebula IC 5070. V1600 Cyg |In the region of the nebula IC 5070. V1608 Cyg |In the region of the nebula NGC 7000. V1610 Cyg |Infrared source CRL 2688, the star of the spectral type V1610 Cyg |F5Ia, associated with a bipolar reflection nebula V1610 Cyg |(the so-called Egg nebula). The northern component of V1610 Cyg |the nebula is 4" to the north from the source. Since 1920 V1610 Cyg |to 1958 the integrated light of this component increased V1610 Cyg |from 15.2m to 13.4b B and after that does not vary [08735]. Light V1610 Cyg |of the faint (16.2m B) southern component (5" to the V1610 Cyg |south from the source) varies by 0.6m B [09176]. The V1610 Cyg |radiation of the nebula is strongly polarized (46%, V1610 Cyg |theta = 106deg in V system). There are C3 absorption V1610 Cyg |features as well as Na, C2, and [S II] emission in the V1610 Cyg |spectrum. Probably the object is a precursor of a V1610 Cyg |planetary nebula [09178]. V1611 Cyg |In the region of the nebula NGC 7000. V1624 Cyg |A var. V1624 Cyg |In 1957 out of a B star turned into Be star. Probably must V1624 Cyg |be referred also to GCAS type. V1661 Cyg |VB A (B 11.14m, 20", 174deg). V1668 Cyg |There are sinusoidal light variations with A(V) = 0.15m V1668 Cyg |and elements Min = 2443767.475 + 0.4392d*E in the V1668 Cyg |descending branch of the light curve after JD2443765 V1668 Cyg |[09179]. Infrared light curves (1.6 - 10 mkm) have a V1668 Cyg |secondary maximum (JD2443815) due to the formation of V1668 Cyg |the dust envelope. At 10 mkm this secondary maximum is V1668 Cyg |brighter than the primary one [09069]. V1669 Cyg |d = 0.036P. V1671 Cyg |Delta(U) = 0.06. V1674 Cyg |VB (B 15m, 5"). V1674 Cyg |The range of combined brightness variation is given. It V1674 Cyg |is not excluded that it is the component B that is V1674 Cyg |variable. Slow variations of mean brightness in the range V1674 Cyg |10.555m - 10.570m B are superimposed by sinusoidal V1674 Cyg |periodikal ones with P1 = 1.3608d (A1 = 0.0037m) V1674 Cyg |and P2 = 0.8055d (A2 = 0.0032m). V1676 Cyg |In the open cluster NGC 6871. V1676 Cyg |ADS 13374 A (B 12.0m, 6.5", 64deg; C 11.0m, 9.5", 28deg V1676 Cyg |D 9.5m, B3V, 11.4", 301deg; E 11.42m, 28.1", 109deg; V1676 Cyg |F 7.36m, B1IA, 35.9", 29deg); SB2 (P = 112.7d). V1696 Cyg |SB1 (Porb = 4.3174d). Epoch of Min brightness is given. V1696 Cyg |The eclipse of the accretion disc around the compact V1696 Cyg |object formed in the outburst of a Supernova in a binary V1696 Cyg |system about 5*10**6 years ago is possible [03619]. V1701 Cyg |In the region of the nebula IC 5070. V1702 Cyg |In the region of the nebula IC 5070. V1703 Cyg |In the region of the nebula IC 5070. V1704 Cyg |In the region of the nebula IC 5070. V1706 Cyg |In the region of the nebula IC 5070. V1707 Cyg |In the region of the nebula IC 5070. V1493 Cyg 10.5"f. V1711 Cyg |In the region of the nebula NGC 7000. V1716 Cyg |In the region of the nebula NGC 7000. V1719 Cyg |Shape of the light curve varies. V1720 Cyg |Min II 7.79. V1721 Cyg |P var.Min I = 2442605.497 + 2.724370d*E (JD2442311 - 928); V1721 Cyg |since JD2442928 - see Table. V1722 Cyg |Min II 14.6? V1726 Cyg |Possible member of an anonimous open cluster. V1727 Cyg |4U 2129 +47. Lx/Lopt ~10. V1727 Cyg |Emissions in the spectrum: NeII lambda 4686A, CIII - NIII V1727 Cyg |lambda lambda 4640 - 50A. V1735 Cyg |In the complex of dark nebulae associated with the V1735 Cyg |open cluster and the nebula IC 5146. Lights up a V1735 Cyg |reflecting nebula. Became brighter by 5m at least V1735 Cyg |from 1952 to 1965. V1737 Cyg |B - V = +3.7. V1738 Cyg |B - V = +5.5:. V1739 Cyg |B - V = +4.5:. V1744 Cyg |Epoch of Max in U system is given. V1746 Cyg |Sometimes P = 0.21d is observed. V1747 Cyg |P > 100d. B - V = +4.0. V1748 Cyg |In the nebula IC 1318a. V1751 Cyg |In the nebula IC 1318c. V1761 Cyg |Close companion? Elements are not certain. V2105 Cyg |Variability type and spectral type (F8Iab:) do not agree. V2121 Cyg |Strong Blazhko effect. V2150 Cyg |Type RR: is also possible. V2174 Cyg |SB, Porb = 225.162d. V2175 Cyg |X-ray source. V2312 Cyg |Erroneously called HD 192776 in [190]. V2324 Cyg |Possible brightening trend over 6 years, maybe due to dissipating V2324 Cyg |dust envelope, plus quicker variations. alf Cyg |VB A (B 11.4m, 75.3", 106deg). tau Cyg |VB A (B 6.44m, G1V, A = 0.88", P = 49.80yr; C 12.20m, tau Cyg |29", 230deg). 0.083d <= P <= 0.125d. tau Cyg |The range of total light variation is given. ups Cyg |VB A (B 10.2m, 15.2", 220deg; C 10.2m, 21.5", 180deg). khi Cyg |VB A (B 10.8m, 158", 254deg). S 6 + %1e (Tc). SiO khi Cyg |maser. P var.Max = 2393559 + 405.88d*E (JD2337150 - 94000); khi Cyg |since JD2394000 - see Table. P Cyg |The appearance of the star was firstly noted in P Cyg |1600, when its brightness was 3m. Since the XVIII P Cyg |century the light of the star varies in the range P Cyg |4.6m - 5.6m vis. Radio source at the millimetre and P Cyg |centimetre wavelengths. Q Cyg |In minimum brightness varies periodically with the Q Cyg |amplitude 0.5m: Max = 2440495 + 54.99d*E; P = 64.81d is Q Cyg |also possible. Mean level of brightness varies in the Q Cyg |range 15.2m - 15.9m B. S Del |VB A (B 56", 342deg). Double maxima are sometimes observed. U Del |Mean brightness var, P = 1100d. According to [08993], the U Del |period value 160d - 180d is more likely than 110d. W Del |d = 0.017P. Min II 9.79. P var. Since JD2433000 - see W Del |Table. The light curve shape var. RZ Del |VB (A var; B var, 17", 137deg) [03771]. TT Del |P var. Since JD2435000 - see Table. TW Del |Delta(m) var (0.5m + 3.4m). TW Del |The light curve resembles that of RV Tau, with Min I and TW Del |Min II; the epoch of Min I is given. TW Del |Min I = 2432171.1 + 118.4d*E (1947 - 1952); TW Del |Min I = 2435386.8 + 115.9d*E (1955 - 1963); during TW Del |1964 - 1970 - see Table. TX Del |P var. P = 6.166585d (JD2428000 - 36600); since TX Del |JD2436600 - see Table. TY Del |Min II 9.8. P var.Min = 2428020.399 + 1.191121d*E TY Del |(JD2428000 - 38000) [00279]; since JD2438000 - see Table. TZ Del |Epoch of Min is given. VV Del |Depth of Min II 0.05m. YY Del |Min II of the depth ~0.05m is possible. P var. YY Del |Min = 2425795.488 + 0.7930856d*E (JD2425000 - 34000) YY Del |[01329]; since JD2434000 - see Table. AL Del |Min II 12.4. BG Del |Min II 13.8. BK Del |P var? BR Del |Emission. BX Del |Delta(S) = 0. BY Del |Min II 11.8. CE Del |[Fe/H] = -0.68. CF Del |The light curve shape var? CH Del |[Fe/H] = -1.23. According to [09037], P = 0.315D. CN Del |Min II 14.6. CR Del |Min II 13.7. CS Del |[Fe/H] = -0.92. CU Del |Abrupt phase chande was noted. CW Del |P var.P = 0.58209d (JD ~2427100), P = 0.58211D CW Del |(JD ~2428800); During JD2429800 - 30600 - see Table. DG Del |The elements should be checked. DK Del |Min II 14.2. DM Del |Min II 8.80. DT Del |Epoch od Min is given. The elements are valid during DT Del |JD2425480 - 6260. DX Del |[Fe/H] = -0.11. EG Del |P var. Max = 2425535.42 + 0.3248545d*E (JD2425478 - 30619) EG Del |[00911]; abrupt change near JD2432578, since then see Table. EI Del |The mean brightness var, P ~600d. EK Del |B - V: +0.29, +0.53. ES Del |Epoch of Max from [03715], [07527] contradict the given ES Del |elements. ET Del |Min II 12.7. EW Del |Min II 15.5. EX Del |Min II 13.3. FI Del |Min II 14.5. FK Del |Min II 14.5. FM Del |Delta(S) = 0. FP Del |[Fe/H] = -1.44. FR Del |Min II 15.3. FT Del |Blazhko effect? GG Del |Min II 12.6. P var? GN Del |P var? Delta(m) var? GY Del |VB B (A = BD +15deg 4134A, SP A - F). HR Del |Porb = 0.170920d. The brightness began to increase on HR Del |JD ~2439653. Waves with maxima on JD2439752 (4.55m), HR Del |2439799 (4.64m), followed by a sharp main Max, flat max on HR Del |JD2439981 (4.09m) and final decline. Radio source. HU Del |mu = 0.685", theta = 79deg. Astrometric binary HU Del |(semiamplitude of deviations 0.118", Porb = 1.52yr). II Del |[Fe/H] = -1.30. IO Del |A single outburst was observed (JD2439378 - 388). IV Del |D ~0.1d. LS Del |Min II 8.76. del Del |(k - b)2 = 0.19. SB2 (Porb = 40.58d; e = 0.7). del Del |Spectra of both SB components show Am features; Fe, Ca, del Del |Sc deficiency, Sr, Y, Zr, Ba, Ce, La, Eu excess. del Del |Both components are DSCT variables; the period of the del Del |main component pulsation is 0.158d, that of the del Del |secondary is 0.134d [07528]. Any of the oscillations may del Del |occasionally dominante in the combined brightness: del Del |according to [07529], Max = 2439338.4444 + 0.135547d*E; del Del |according to [07530], P = 0.154991d. R Dor |VB A (B 11.9m, 34", 10deg; C 11.0m, 35", 130deg, 1933). R Dor |H2O, SiO, HC3N emission. S Dor |VB A (B 12.1m, 13"). The member of the large magellanic S Dor |cloud. In the cluster NGC 1910 and a diffuse nebula. S Dor |One of the absolutely brightest stars. Deep Min: 1891, S Dor |1900, 1930, 1940, 1955, 1964. T Dor |VB A (B 12.0m vis, 5", 13deg.) V Dor |At the edge of the Large Magellanic Cloud. RR Dor |In the region of the Large Magellanic Cloud. Min II 14.5. RW Dor |In the region of the Large Magellanic Cloud.Cloud RW Dor |non-member. P var [09036]. Min II 11.2. RX Dor |In the region of the Large Magellanic Cloud. Cloud RX Dor |non-member? SW Dor |In the region of the Large Magellanic Cloud. SW Dor |Cloud non-member. P var [09036]. SX Dor |In the region of the Large Magellanic Cloud, SX Dor |Cloud non-member. Delta(m) var. SY Dor |In the region of the Large Magellanic Cloud. SY Dor |According to [09036], variability is doubtful. SZ Dor |In the region of the Large Magellanic Cloud, cloud SZ Dor |non-member. TY Dor |In the region of the Large Magellanic Cloud, cloud TY Dor |non-member. UU Dor |In the region of the Large Magellanic Cloud,cloud UU Dor |non-member. UV Dor |In the region of the Large Magellanic Cloud,cloud UV Dor |non-member. UX Dor |In the region of the Large Magellanic Cloud, cloud UX Dor |non-member. XX Dor |In the region of the Large Magellanic Cloud, cloud XX Dor |non-member. [Fe/H] ~-1.3. ZZ Dor |In the region of the Large Magellanic Cloud, cloud ZZ Dor |non-member. AA Dor |d = 0.02P. Min II 11.21. alf Dor |VB A (B 4.3m, A = 0.2125", P = 13.00yr.) alf Dor |The range of combined brightness variations is given. bet Dor |P var. Current elements are given. T Dra |ADS 10937 A (B = UY Dra, optical, 16", 222deg). U Dra |P var. Mean elements are given. W Dra |P var. Max = 2416748 + 257.11d*E (JD2416750 - 21390); W Dra |Max = 2430826 + 262.11d*E (JD2421390 - 30820); W Dra |Max = 2439962 + 268.87d*E (JD2430820 - 40490); W Dra |since JD2440490 - see Table. Y Dra |According to visual observations, 7.8m - 15.0m. Z Dra |Min II 11.0. P var. Min = 2430973.314 + 1.3574176d*E Z Dra |(JD2428460 - 33300); Min = 2433268.708 + 1.357440d*E Z Dra |(JD2433300 - 43500); since JD2443500 - see Table. RR Dra |d = 0.015P. Min II 10.1. P var. Before JD2439000 RR Dra |Min I = 2433390.458 + 2.83123d*E [01001]; RR Dra |since JD2440000 - see Table. RS Dra |During JD2436012 - 37584 P = 145.3d. RS Dra |Delta(m) and the light curve share vary strongly. RW Dra |P var. Mean elements are given. RW Dra |Composite Blazhko effect; RW Dra |Pi = 93.95P = 41.61d; Pi1 = 280P; Pi2 = 6140P; Pi3 = RW Dra |3400P [01585]. 0.11P <= M - m <= 0.32P. Delta(S) = 3. RX Dra |Min II 10.3, d II = 0.009P. RZ Dra |Min II 10.38. P var. Min = 2429448.787 + 0.55087668d*E RZ Dra |(1907 - 1968) [03822]; since 1968 - see Table. SU Dra |P var. Before 1955 Max hel = 2420605.762 + SU Dra |0.66041890D; since 1955 - see Table. [Fe/H] = -1.39. SW Dra |Delta(S) = 3.5. SX Dra |d = 0.035P. Min II 10.0. P var. Min I = 2432273.276 + SX Dra |5.1692d*E (JD2432000 - 38000); since JD2442000 - see Table. TT Dra |P2 = 198d. TW Dra |ADS 9706 A (B 9.5m vis, 23deg, 3.6"). d = 0.02P; TW Dra |Min II 8.1. P var. Min I = 2433888.452 + 2.806870d*E TW Dra |(JD2433000 - 40000) [03825]; since JD2440000 - mean TW Dra |elements in the Table. TX Dra |Mean magnitude var, P2 = 654d. UU Dra |Mean magnitude var, P2 = 960d. UX Dra |According to [09086], the light curve may correspond UX Dra |to the type E; SB, P ~340d. UZ Dra |d = 0.01P; Min II 10.6. Possibly P = 1.65d [03827]. VW Dra |According to photoelectric observations, 6.28m - 6.32m V. WW Dra |Nonlinear term: -4.98d*10**(-9)*E2. WW Dra |ADS 10152A (B 9.67m, 8.2", 5deg). Depth of Min II 0.08m. WZ Dra |Delta(m) var strongly. XY Dra |Min II 13.7. XZ Dra |P var. Before JD2438000 Max = 2427985.648 + 0.4764944d*E XZ Dra |[00188]. Epochs after JD2438000 are represented dy the XZ Dra |elements in the Table only on average. Blazhko effect; XZ Dra |according to [01474], Pi = 78d. [Fe/H] = -0.57. ZZ Dra |P var. Max = 2434509 + 274.5d*E (JD2416350 - 34600); since ZZ Dra |JD2437100 - see Table. AE Dra |Delta(S) = (4). AF Dra |VR var; SB? AG Dra |A soft X-ray source. Elements in the Table represent AG Dra |maxima in U band in 1974 - 1979 [09113]. AI Dra |Min II 7.16, D II = 0.17P. AP Dra |Twice shorter period is possible. AQ Dra |Hbeta spectral line is probably filled in by emission. AR Dra |Min II 11.63. AS Dra |mu = 0.486", P = 289deg. SB. Delta(m) var. AS Dra |Large spatial velocity. The brightness AS Dra |varies with the phase of the orbital motion. Phases AS Dra |of Max and Min vary from cycle to cycle. The Table AS Dra |gives Porb [03075] and the epoch of the conjunction AS Dra |(G4 - star is behind). AW Dra |P var. since JD2430500 - see Table. AX Dra |Min II 11.0. BE Dra |Min II 11.5. The spectral type is late B. BH Dra |ADS 12019A (B Am, 9.25m, 10.8", 58deg). Min II 8.58. BK Dra |P var.Max = 2415150.817 + 0.592019d*E (JD2414900 - 16150) BK Dra |[00001]; since JD2416940 - see Table. BK Dra |Delta(S) = 8 in Max light. BP Dra |Min II 14.7. BS Dra |Min II 9.84. BV Dra |ADS 9537 A (B = BW Dra, 16.3", 358deg, 1980; C 12.69m). BV Dra |Min II 8.40. BW Dra |ADS 9537 B (A = BV Dra; C 12.69m). Min II 9.02. BY Dra |SB2 (Porb = 5.9750998d, e = 0.36). mu = 0.365", P = 150deg. BY Dra |Quasiperiodic variability : BY Dra |DM var, P var, (differential rotation), phase jumps. BY Dra |Flares up to Delta(U) = 1.07m. CM Dra |VB A (B SP = DC, 15.7m pg, 25.7", 22deg, common mu). CM Dra |mu = 1.619", p = 317deg, pi = 0.068", V nu = -118.6km/s. CM Dra |Min II 13.63. BY type variability: Delta(M) ~<= 0.05mV, CM Dra |P ~Porb. Flares: Delta(m) ~0.05. CR Dra |mu = 0.50", p = 168deg, pi = 0.048". CX Dra |SB, Porb = 6.69612d (with this period Delta(V) = 0.04m). CX Dra |Long-term cyclic variations: P ~2400d, Delta(V) ~0.2m. CX Dra |Flares ~0.1m. An X-ray source; the reflection effect is CX Dra |observed. DE Dra |d = 0.017P. DG Dra |Depths respective to Max I (D = 0.25); Min II 0.17m; DG Dra |Max II 0.01m. DK Dra |Porb = 64.44d. DK Dra |Epoch of Min is given. Both components show H and K CaII DK Dra |in emission. DL Dra |VB A (B 9.2m, 3.9", 318deg, 1982). P1 = 0.0825d, A1 = DL Dra |0.028m; P2 = 0.0837d, A2 = 0.026m. DN Dra |P = 109S. mu = 0.32", P = 153deg. kap Dra |IR excess. phi Dra |ADS 11311 (Delta(m) = 1.7m, 0.3", 288deg, 1967). A:SB, P = phi Dra |26.768d. The epoch of Max U light is given. S Equ |Min II 8.11. P var. Before JD2427000 Min = S Equ |2423746.490 + 3.4360050d*E [01140]; Min = S Equ |2437968.345 + 3.436072d*E (JD2427000 - 41000) S Equ |[03432]; since JD2441000 - see Table. S Equ |Gaseous streams; in Min light Halpha is in emission. W Equ |Min II 12.4. P var. Z Equ |A nearby star: 12.1m. RT Equ |P var strongly. RW Equ |Strong Blazhko effect. RZ Equ |Min II 12.2:. SU Equ |Min II 16.4. SV Equ |Depth of Min II 0.16m. SW Equ |Min II 15.6. gam Equ |ADS 14702A (B 11.6m, 2", 268deg; C 12.6m, 48", optical). gam Equ |The Table gives the period of oscillations. Data on the gam Equ |periodicity of the rotational variability of light, gam Equ |spectrum and magnetic field are contradictory gam Equ |(17.492d, 314d, 1785.7d, 72yr). V Eri |Mean magnitude var, P2 = 1209d. W Eri |SiO, OH, H2O maser. Z Eri |P2 = 746.4d. RU Eri |Min II 9.62. RX Eri |[Fe/H] = -1.32. RY Eri |d = 0.025P. RZ Eri |d = 0.018P. The depth of Min II 0.04m pg. SV Eri |[Fe/H] = -1.83. P var. P = 0.71365272d (JD2414000 - 21000); SV Eri |P = 0.71370172d (JD2421000 - 26000) [00862]; SV Eri |Max = 2426590.319 + 0.7137406d*E (JD2426000 - SV Eri |34000) [09195]; since JD2434000 - see Table. TT Eri |(B - V)Max = +0.255m. TV Eri |(B - V)Max = +0.53m. TZ Eri |d = 0.015P. P var. Min = 2426066.198 + 2.606097d*E TZ Eri |(JD2426000 - 33500) [01490]; since JD2438200 - see Table. UX Eri |Min II 11.01. P var? Before JD2438500 Min I = UX Eri |2434368.570 + 0.4452820d [02494]; since JD2438500 - see UX Eri |Table. UY Eri |The shape of the light curve var. [A/H] = -1.6. VW Eri |Alternating P1 = 83.4d, P2 = 93.3d. Halo population. WW Eri |Min II 11.2. WX Eri |The depth of Min II 0.22m. The primary component var, WX Eri |DSCT:, P1 = 0.16454d, P2 = 0.13721d. YY Eri |Min II 8.72. P var. Min I = 2433617.5198 + 0.321496212d*E YY Eri |(JD2433000 - 41500) [03850]; since 2441500 - see Table. YY Eri |X-ray source. ZZ Eri |Min II 14.4. AN Eri |Min II 14.9. AO Eri |d = 0.04P. AS Eri |Min II 8.42. X-ray source. BB Eri |(k - b)2 = 0.13. BC Eri |Min II 11.26:. BK Eri |Delta(S) = 8. P var. BL Eri |The elements should be checked. BM Eri |P > 20000d; D = 321d; d = 270d. BM Eri |Only one Min was observed. Outside Min, according to BM Eri |[05828], Delta(V) = 0.2m, Max = 2440643.0 + 30d*E. BQ Eri |Min II 10.9. BV Eri |Min II 8.42. dII = 0.06P. BW Eri |Min II 9.72. BY Eri |(k - b)2 = 0.06. BZ Eri |Min II 9.21. CC Eri |SB. mu = 0.310", P = 169deg, Pi = 0.083". CC Eri |Photometric P is close to Porb. X-ray source. CI Eri |VB (9.9m, 11.2m, 2", 106deg). CO Eri |Min II 9.1. CS Eri |(k - b)2 = 0.03. CT Eri |Min II 10.27. CW Eri |Min II 8.86, DII = 0.10P. DL Eri |P0 - see Table; P1 = 0.118795d [09206]; P2 = 0.0968d [09207]. DM Eri |ADS 3380 (5.1m, 5.4m, 0.3", 161deg). DM Eri |Duplicity was observed only in 1877 and 1923. DO Eri |Epoch of Min is given. Oscillations with P ~6.14 Min, 7 DO Eri |different frequencies have been found. Beat phenomenon, DO Eri |PB = 12.25d +-0.47d. Max of the oscillation amplitude DO Eri |almost coincides with Max of the magnetic field, the DO Eri |amplitude varies with Prot. Combined amplitude of DO Eri |oscillations 0.062m B. DS Eri |Min II 10.3. P var. Min = 2423147.25 + 0.827737d*E DS Eri |(JD2414869 - 23150); during JD2423150 - 31320 - see Table. DW Eri |ADS 3409 B (A 6.72m, G8III; B 9", 317deg). DY Eri |ADS 3093 C (A 4.43m V, K1V; B 9.51m V, DA, 82", DY Eri |105deg; BC A = 7", Porb = 252.1yr). mu = 4.05", P = 212deg. DY Eri |X-ray source. DZ Eri |Epoch is given for Max (y), Min (He I). DZ Eri |P = 3.67d is possible. EF Eri |2A0311 - 227. VB A (B 15.8m, 18", 260deg). mu alpha = EF Eri |+0.147", mu delta = -0.070". EF Eri |Epoch of narrow Min in IR light is given. The complex EF Eri |phenomenon of eclipses is described in [04041]. EF Eri |Oscillations with P ~20.2 and 13.7 Min. [09211]. Flickering. EG Eri |Epoch of Min in Y light is given. EH Eri |ADS 3305 A (B 10.8m, 1.45", 60deg, 1917). HV Eri |Type RRC: is also possible. gam Eri |ADS 2904 A (B 12.4m, 53", 242deg). lam Eri |Shell features are sometimes present in the spectrum. nu Eri |SB? P2 = 0.1735079d. Beat effect. omi 1 Eri |P0 - see Table. P1 = 0.1291d. tau 4 Eri |ADS 2472 A (B 9.9m, 6", 288deg; C 11m, 40", 99deg). tau 9 Eri |SB1 (Porb = 5.954d). P = 1.2135d is not excluded. S For |VB (9.2m, 9.3m, 0.28", 358deg, 1964). S For |Found unusually bright only on one night S For |by three experienced observers in europe; harvard S For |photographs of the same night show it in normal brightness. V For |(B - V)Max = +0.26. W For |Min II is observed. RX For |(k - b)2 = 0.06. RY For |(B - V)Max = +0.535. SS For |(k - b)2 = 0.09. SW For |Delta(S) > 10:. SY For |SB2 (M + pec(eq)). TZ For |SB2. Possible P values: TZ For |37.805d; 44.18d; 50.46d; 75.61d. DI = 1d. R Gem |VB A (B 11.4m pg, 173", 200deg, 1910). S 3.5/6e- S 6.5/6-. S Gem |VB A (B 11.1m, 70", 122deg). T Gem |S 3/4e. U Gem |Min = 2437638.82685 + 0.17690602d*E + 5.4d*10**(-12)*E**2 U Gem |[09215]. Depth of Min 0.5m - 1.0m. U Gem |Spectrum description [09216]. V Gem |P var. Max = 2407750 + 276.2d*E (JD2407700 - 15500); V Gem |Max = 2415729 + 278.3d*E (JD2415600 - 21600); Max = V Gem |2421839 + 269.8d*E (JD2421700 - 26500) [00458]; Max = V Gem |2432580 + 281.3d*E (JD2427500 - 32600); Max = V Gem |2434739 + 269.8d*E (JD2432600 - 35800); V Gem |since JD2435800 - see Table. W Gem |P var. Max = 2429815.990 + 7.914553d*E (JD2413200 - W Gem |31700); since JD2431700 - see Table. [A/H] = 0.2. W Gem |There is possibly faint blue companion. RR Gem |P var. Max = 2415219.734 + 0.39729235d*E RR Gem |(JD2412000 - 18000); Max = 2418278.900 + 0.39727274d*E RR Gem |(JD2418000 - 21000); Max = 2422865.229 + RR Gem |0.39724027d*E (JD2421000 - 25000) [09217]; Max = RR Gem |2427150.267 + 0.3972596d*E (JD2426200 - 27850); RR Gem |Max = 2434806.289 + 0.3973103d*E (JD2428200 - 34900) RR Gem |[02392]; since JD2436000 - see Table. Blazhko effect, RR Gem |PB = 48d [03618], PB = 37d [09221]. Delta(S) = 3. RW Gem |VB A (B 11.04m, 20", 105deg; C 11.84m, 100", 120deg). RW Gem |Min II 9.74; d = 0.02P. RX Gem |VB A (B 12.65m, 45", 215deg). Min II 9.28; d = 0.004P. RX Gem |P var. Min I = 2417970.0 + 12.20868d*E (JD2415000 - 27500) [07534]; RX Gem |since JD2427600 - see Table. RX Gem |There is a square term in the elements given in the Table: RX Gem |+2.25d*10**(-7)*E**2. Luminous gaseous ring surrounds the RX Gem |primary component of the system [07535]. RY Gem |VB A (B 12.30m, 45", 240deg). Min II 8.75; d = 0.023P. RY Gem |P var. Min I = 2418015.333 + 9.300876d*E RY Gem |(JD2418000 - 33000) [08653]; since JD2433000 - see Table. RY Gem |Component of A type is surrounded by a luminous gaseous RY Gem |ring. RZ Gem |VB. P var. Max = 2429632.453 + 5.529716d*E RZ Gem |(JD2415000 - 32400); since JD2432400 - see Table. SS Gem |9.9m <= Min II <= 10.7m. SU Gem |P var. Min I = 2429204 + 50.12d*E (JD2429200 - 355) SU Gem |[00310]; Min I = 2437772.5 + 50.39d*E (JD2437739 - SU Gem |39850); Min I = 2439856.6 + 50.10d*E (JD2439850 - SU Gem |40680); since JD2440680 - see Table. SU Gem |Mean brightness varies with the elements: SU Gem |Min = 2437953 + 680d*E; M - m = 264d. SU Gem |Amplitude of shortperiodical variations is 0.3m - 0.9m. SW Gem |Min brightness epoch is given. SX Gem |Min II 11.3; d = 0.05P:. TX Gem |Depth of Min II 0.04m; d = 0.017P:. UV Gem |VB A (B 19.5m, 7", 285deg). WW Gem |Min II 10.3. WY Gem |May be an eclipsing system similar to VV Cep. Atmospheric WY Gem |eclipse began probably in 1960 - 61, the mean phase of it WY Gem |being in 1968 [05730]. Variable magnetic field [01591,04498]. WY Gem |Intrinsic variability of blue component is also possible WY Gem |[07536]. YY Gem |VB C (A 1.99m, B 2.85m, a = 6.06", P = 306.3 y; C 73", YY Gem |165deg, 1925); mu alpha = -0.0154s, mu delta = -0.108". YY Gem |Min II 9.59; Min II - Min I = 0.50P; D = 0.000P. X-ray YY Gem |source. P const [08655]. Both components are probably YY Gem |UV Cet type variables. Flare amplitude in the integrated YY Gem |light of the system reaches 0.3m V, or 1.8m U [09227]. AA Gem |[A/H] = 0.0. AC Gem |Min II 11.3. P var. Min I = 2433649.30 + 1.661795d*E AC Gem |(JD2415000 - 36000) [01530]; since JD2430100 - see Table. AF Gem |VB A (B 14.8m, 2", 0deg). Min II 10.67. AF Gem |There is a square term in the elements given in the Table: AF Gem |-1.71d*10**(-10)*E**2. AH Gem |Min II 14.8:. AI Gem |Min II 14.0. AL Gem |Min II 9.85. AN Gem |Min II 13.3:; d = 0.037P. AU Gem |OH emission. AV Gem |Min II 12.8:. AY Gem |Min II 10.9. AZ Gem |Min II 12.4. BB Gem |VB A (B 12m, 25", 270deg). BP Gem |P var. Max = 2434120 + 243.9d*E (JD2418700 - 36600); BP Gem |since JD2436600 - see Table. BT Gem |Min II 14.0:. CI Gem |UG? CM Gem |Min II 15.0. DL Gem |VB A (B 13.1m, 18", 180deg). DN Gem |VB A (B 13.5m, 12", 16deg; C 12.0m, 80", 99deg). DP Gem |Min II 14.0. RRC? P = 0.2792d? DX Gem |P var. Max = 2433182.876 + 3.136226d*E (JD2425000 - DX Gem |34000); Max = 2435554.199 + 3.136955d*E DX Gem |(JD2434000 - 36500) [08300]; since JD2436500 - see Table. EF Gem |P var. Min = 2428108.49 + 6.10222d*E (JD2428500 - EF Gem |42800) [00407]; since JD2442800 - see Table. EL Gem |Min II 13.6. EN Gem |Min II 13.8. EW Gem |P var. Max = 2428495.686 + 0.523750d*E (JD2428100 - 30780); EW Gem |since JD2430780 - see Table. EY Gem |Min II 13.0. FT Gem |Min II 14.1. GP Gem |Min II 13.5. GR Gem |15.6 <= Min II <= 15.9. GW Gem |Min II 10.68. GX Gem |Min II 11.3. GZ Gem |P = 1.225290d? HH Gem |Min II 13.8. HR Gem |Min II 11.7. HY Gem |Min II 17.5. II Gem |P = 223d? IP Gem |Min II 14.5. IR Gem |In supermaxima there are superhumps with P = 102 Min IR Gem |[09232]. IZ Gem |D >= 0.24d. KN Gem |The minor planet (123) Brunhild. KQ Gem |Min II 14.6. KU Gem |d = 0.05P. KV Gem |Epoch of Min of brightness is given. EW KV Gem |type is possible according to the spectrum [09037]. KZ Gem |The cycle may be 129d. LM Gem |d = 0.02P. LX Gem |Red. MO Gem |Red. MP Gem |VB. MU Gem |Min II 14.9. MZ Gem |Min II 16.7. NQ Gem |In the spectrum of the carbon NQ Gem |star the hydrogen emission lines and ultraviolet NQ Gem |continuous emission appeared in February 1970 [06348]. NY Gem |HD 47396 (Pec) = S 5438 = CSV 798 = CSV 6468. NY Gem |In the chart in [00156] the position of the variable is NY Gem |wrong. OS Gem |Oscillations with OS Gem |the period P1 given in the Table are superimposed OS Gem |by oscillations with the period P0 = 0.070d and smaller OS Gem |amplitude. P1/P0 = 0.78. V0345 Gem |The variability may be due to the fainter (B) component. zet Gem |VB A (B 11.46m, 87", 84deg; C 7.56m, 97", 350deg). P var. zet Gem |Max = 2410640.42 + 10.15477d*E (JD2394600 - 2407150); zet Gem |Max = 2422366.187 + 10.15288d*E (JD2407150 - 22300); zet Gem |Max = 2426802.918 + 10.15172d*E (JD2422300 - 34500) zet Gem |[02392]; since JD2434500 - see Table. zet Gem |All the observations are satisfied also by the zet Gem |elements: Max = 2443785.444 + 10.150135d*E - zet Gem |5.24d*10**(-7)*E**2 [09029]. zet Gem |May by a DCEPS type variable. eta Gem |VB A (B 8.8m, GO III - IV, 1.60", 269.4deg, 1977). SB1 eta Gem |(P = 2983d [09236]). Epoch of Min brightness is given. eta Gem |The deepest minima (corresponding to the middles of the eta Gem |descending branches of the radial velocity curve) are eta Gem |satisfied by the elements: Min = 2429355 + 2984d*E eta Gem |[01551]. mu Gem |VB A (B 9.8m, 122", 141deg). sig Gem |VB A (B 10.8m, 182", 316deg); SB1 (P = 19.603d [09238]). sig Gem |There is a Min II on the light curve; Min II sometimes sig Gem |disappears and sometimes becomes deeper then Min I. sig Gem |Min II - Min I = 0.5P. U Gru |Depth of Min II 0.05m. d = 0.011P. W Gru |P var. Nonlinear term: +7.84d*10**(-9)*E**2. Min II 10.0. X Gru |d = 0.008P. Min II 10.69. P var. X Gru |Current elements are given. Z Gru |Delta(S) = 12:. Z Gru |The shape of the light curve and P are strongly variable. RS Gru |(k - b)2 = 0.22. RT Gru |(k - b)2 = 0.02. Blazhko effect. RV Gru |(B - V)Max = +0.93. Min II 11.4. RW Gru |Delta(S) = 10. Blazhko effect. RX Gru |Min II 10.7. RY Gru |Superposition of irregular variations? RY Gru |During JD2434513 - 517 precalculated minima were not RY Gru |observed. RZ Gru |A description of light changes [02809]. UW Gru |[Fe/H] = -1.6. VW Gru |P >= 260d? VY Gru |P > 160d. VZ Gru |RR type is also possible. AK Gru |Elements should be checked. AP Gru |P var. Mean elements JD2427992 - 36848 - see Table. AP Gru |during JD2434250 - 36848 Max = 2434337.337 + 0.5082945d*E. AR Gru |Min II 10.6. AV Gru |P >= 160d is possible. AW Gru |Min II? JD2436818. BC Gru |Min II 10.3. RRC type is possible. BD Gru |Min II 14.9. BH Gru |Min II 15.2:. pi 1 Gru |VB A (B 10.9m, G0V, 2.7", 202deg). T Her |VB A (B 10m, 67", 321deg). U Her |SiO, OH, H2O maser. W Her |ADS 10121 A (B 14.2m, 6", 334deg). X Her |P2 = 746d. Z Her |VB A (B ro > 10"). Min II 8.18. Z Her |nonlinear term: -6.19d*10**(-10)*E**2. RU Her |SiO maser. The spectrum in Min RU Her |light is composite; a companion? [03502]. RX Her |Min II 7.74. SW Her |B - V; +0.12, +0.40. P var. Before 1921 Max = SW Her |2416687.018 + 0.4928864d*E. SX Her |[Fe/H] = -1.8. SY Her |On period variations see [08699]. SZ Her |Min II 10.10. P var. Min = 2430766.8390 + 0.818096d*E + SZ Her |0.0165d*sin(0.010465deg*E + 180deg) [05749]. SZ Her |The Table gives current elements satisfac - SZ Her |tory after JD2438000. TT Her |Min II 9.89. The light curve shape var. TT Her |P var. Before JD2430000 Min = 2425433.627 + TT Her |0.9120846D [02389]; Min = 2434525.2572 + 0.9120800d*E TT Her |(JD2430000 - 40000) [03504]; since JD2440000 - see Table. TU Her |d = 0.022P. P var. Before JD2435000 Min = TU Her |2424381.416 + 2.2671303d*E - 854d*10**(-11)*E**2 [09240]; TU Her |Min = 2437462.3909 + 2.2669718d*E (JD2435000 - TU Her |38000) [09241]; Min = 2443324.70097 + 2.2669385d*E TU Her |(JD2438000 - 44000) [08593]; since JD2444000 - see Table. TW Her |[Fe/H] = -0.47. TX Her |Min II 8.97, DII = 0.11P. P var; TX Her |periodic term: +0.0081d*sin(0.042deg*(E + 7255)). UU Her |[Fe/H] = -1.27. UU Her |There was alternation of periods 90d and 71d UU Her |[00310]; the period 45d [03507] was also noted. UU Her |During JD2443611 - 44161 - see Table. Epoch of Min is given. UX Her |Min II 9.11. P var. Before JD2429000 Min = UX Her |2419876.467 + 1.5488598d*E [00279]; Min = UX Her |2429987.420 + 1.5488513d*E (JD2429000 - 38000) UX Her |[03671]; since JD2438000 - see Table. VW Her |VB A (B 17.3m, 18", 120deg. VX Her |Delta(S) = 5. P var; nonlinear term: VX Her |-0.00745d (E:10000)**2. According to [03369], VX Her |a member of an eclipsing binary system. VZ Her |[Fe/H] = -0.9. P var. P = 0.44031880d (JD2415000 - VZ Her |22000) [05738]; Max = 2425004.4590 + 0.44032394d*E VZ Her |(JD2422000 - 27000); Max = 2425004.4456 + VZ Her |0.44032631d*E (JD2427000 - 36000) [03506]; VZ Her |since JD2436000 - see Table. WW Her |VB A (B 15.6m, 7.4", 148.5deg, white). WX Her |Twice longer P is not excluded. AC Her |P var. AC Her |The Table gives current elements valid since JD2442000. AC Her |Mean P = 75.4619d [01754]. The magnitude in AC Her |Max varies with Delta(m) = 1.6m [00368]. AD Her |VB A (B 11.97m, 5", 189deg). d = 0.033P. Min II 9.79. AF Her |P var. Before JD2426950 P = 0.630336d; AF Her |since JD2426950 - see Table. AF Her |The shape of the light curve var. AG Her |P var. Max = 2422935.584 + 0.6494378d*E AG Her |(JD2418210 - 26952); since JD2426952 - see Table. AH Her |Porb = 5.9d:. Oscillations during outbursts: AH Her |24s <= P <= 39s, Delta(m) <= 0.003m [09251]. AH Her |Flicckering in Max And Min up to 0.4m in 2 - 8 minutes AH Her |[09252]. AK Her |ADS 10408 A (B 12.0m, 5", 323deg). Min II 8.64. AK Her |Min II - Min I = 0.505P. dII = 0.07P. P var. Before AK Her |JD2421200 Min = 2421200.549 + 0.42152207d*E; Min = AK Her |2421200.549 + 0.42152083d*E (JD2421200 - 24950); AK Her |Min = 2424949.555 + 0.42152061d*E (JD2424950 - AK Her |30000) [01760]; Min = 2430939.368 + 0.42152362d*E AK Her |(JD2430000 - 41500); since 2441500 - see Table. AK Her |The shape of the light curve var. AM Her |3U 1809 +50. Lx(soft)/Lopt ~15. AM Her |Emissions of H and KCaII, H, HeI, HeII, etc. AM Her |In the spectrum. Epoch of Min I in V light is given. AM Her |The period shows complex variations. The phase of Min I AM Her |in U light is 0.30p, in B 0.15P, in R 0.05P. Min I is AM Her |probably due to an eclipse of a hot spot and the gas flow AM Her |near the surface of the white dwarf by the white dwarf AM Her |itself. The depth of Min I is up to 0.7m. Min II with the AM Her |depth up to 0.4m (sometimes absent), Min II - Min I = 0.55P. AM Her |Min II coincides in phase with the X-ray eclipse. AM Her |High and low states (b ~13.0m and B ~15.0m on average); AM Her |in the high state there are variations with Delta(m) ~0.3m AM Her |on the time scale >= 200d; the duration of low states is AM Her |130d - 700d [09258] or less. During low states the AM Her |depth of minima is small. Flickering up to 0.8mV in AM Her |several minutes or dozens of seconds; X-ray flickering AM Her |on the time scale of ~10s not correlating with AM Her |optical flickering. The magnetic field ~1*10**7 G at AM Her |the equator, ~2*10**7 G on poles. Variable circular AM Her |(from +3% to -9%) and linear (up to 7%) polarization. AM Her |IR excess at lambda 10 mkm. AP Her |P var strongly. P = 10.400d (JD2415000 - AP Her |19000:); P = 10.3970d (JD2423700 - 24700:); P = AP Her |10.4260d (JD2424700 - 25300); P = 10.4338D AP Her |(JD2425800 - 27000); P = 10.3945d (JD2427000 - 27400); AP Her |P = 10.4277d (JD2433000 - 33850); P = 10.3898d AP Her |(JD2433850 - 34850); P = 10.4209d (JD2434850 - 35600); AP Her |P = 10.3715d (JD2435600 - 37200); AP Her |DURING JD2437200 - 43800 - see Table. AP Her |The light curve shape var. [A/H] = -0.8. AR Her |P var in a complicated way. Max = AR Her |2424794.274 + 0.4700234d*E (1905 - 1954) [06535]; AR Her |Max = 2439692.683 + 0.469975d*E (1954 - 1967) [05274]; AR Her |since 1967 - see Table. AR Her |Blazhko effect, Pi = 31.5489d [03555], AR Her |Delta(m) var (0.9m -: 1.8m pg) [02168], (M - m) var. AR Her |Delta(S) = 6. AT Her |The star is bright on one plate (JD2418209). AT Her |Besides that, 11.8m - 12.25m. AW Her |VB A (B 10" - 20"). d = 0.03P. BB Her |P var. P = 7.507696D (JD2418924 - 30700); BB Her |since JD2430700 - see Table. [A/H] = +0.3. BC Her |P var. Before JD2432000 Min = 2426242.372 + BC Her |3.08752d*E [09262]; since JD2436000 - see Table. BD Her |P var. P = 0.4739135d (JD2426540 - 29620); P = BD Her |0.4739057d (JD2429620 - 30570); Max = 2430495.404 + BD Her |0.4739126d*E (JD2430570 - before 1948) [09263]; BD Her |since 1948 - see Table. Delta(S) = 0.8. BL Her |P var. P = 1.3074604d (JD2415000 - 35000); BL Her |since JD2435000 - see Table. Another possible BL Her |representation: Max = 2434999.402 + 1.307457d*E - BL Her |3.9d*10**(-10)*E**2 (JD2415000 - 42000). [Fe/H] = 0.0. BO Her |d = 0.015P. Min II 10.8. P var? CC Her |P var. Min = 2426120.415 + 1.7340314d*E (JD CC Her |2425790 - 31265); Min = 2431265.288 + 1.7340460d*E CC Her |(JD2431265 - 36000) [02389]; Min = 2439668.342 + CC Her |1.73398d*E (JD2436000 - 39600); since JD2439600 - see CC Her |Table. CD Her |The chart in [06286] is wrong. CE Her |[A/H] = -1.8. CK Her |P var? Max = 2429231.234 + 0.519201d*E (JD2429231 - CK Her |877) [00332]; during JD2436041 - 37955 - see Table. CO Her |P2 = 600d. Sometimes does not vary for 150d. CP Her |Superimposed waves, 50d - 100d. CT Her |The depth of min II 0.05m. P var. CT Her |Min = 2430904.431 + 1.786337d*E (JD2426480 - 35000) CT Her |[03567]; Min = 2439355.666 + 1.7863645d*E CT Her |(JD2435000 - 39500) [00001]; Min = JD2441499.3307 + CT Her |1.7863891d*E (JD2439500 - 42500) [08593]; CT Her |since JD2442500 - see Table. DE Her |P var. Max = 2425754 + 171.2d*E (JD2425754 - 30890); DE Her |Max = 2430889 + 175.3d*E (JD2430890 - 36150); DE Her |during JD2436150 - 38140 - see Table. DF Her |Elements are valid since JD2425900. DH Her |d = 0.024P:. Min II 9.5. DI Her |Min II 8.95, DII = 0.03P, Min II - Min I = 0.77P (1966 - DI Her |1978). Apsidal motion: P = 29000yr +- 4000yr; DI Her |Min II = 2442241.4602 + 10.5501751d*E. DI Her |A considerable discrepancy between the observed and DI Her |the theoretical rate of apsidal motion. DK Her |P var. DL Her |Blazhko effect, Pi = 33.6d, 11.0m <= m Max <= 11.3m. P var. DL Her |Delta(S) = 5. DO Her |Close to V362 Her. DQ Her |VB A (B 18.17m, F, 3.5", 132deg, optical?). DQ Her |Nebula, R = 10.5" (Halpha, 1981). DQ Her |After the main Max of the Nova a deep DQ Her |Min 13.0m (JD2426925) and a flat secondary Max DQ Her |6.7m (JD2427065) were observed. DQ Her |Eclipsing variability: DQ Her |14.61m - 18.08m, Min HeI = 2434954.9445 + 0.193620877d*E DQ Her |[09280]. D = 0.20P, d = 0.000P. DQ Her |The light curve shape and Delta(M) var. DQ Her |Oscillations: Max HeI = JED2434954.785868 + DQ Her |8.22521640d*10**(-4)*E - 2.8048d*10**(-16)*E**2 DQ Her |[08722], 0 <= Delta(m) <= 0.08m. DQ Her |Polarization changes with double oscilation period. DQ Her |Flickering: Delta(m) = 0.15m. DY Her |P var, nonlinear term: -18.6d*10**(-13)*E**2. EI Her |Red. EN Her |P var. Before JD2427000 P = 160d. ES Her |Min II 13.7. ET Her |The elements are valid earlier than JD2427200 EX Her |Red. EZ Her |The elements are valid earlier than JD2427400. FN Her |P var? FW Her |Min II 14.6. FY Her |According to the spectrum, EW type is possible. GL Her |P var? GU Her |d = 0.010P. Min II 11.8. Min II - Min I = 0.513P. GV Her |[Fe/H] = -1.41. P var. Max = 2427543.360 + GV Her |0.2914606d*E (JD2427543 - 29728) [00152]; GV Her |during JD2436041 - 38170 - see Table. GY Her |P var. Max = 2428219.623 + 0.524347d*E (JD2428219 - GY Her |727) [00152]; during JD2436370 - 38170 - see Table. HS Her |d = 0.025P. Min II 8.63. P var; since JD2438240 - see HS Her |Table. Apsidal motion: Pi ~130yr [06538]. HV Her |d = 0.008P:; Min II 12.9:. HZ Her |Her X-1 = 4U 1656 + 35. Lx/Lopt = 2 - 60. HZ Her |The Table gives elements for light minima due HZ Her |to eclipsing variability and the reflection effect. Min I HZ Her |coincides with the X-ray eclipse. Shallow Min II may HZ Her |be present. The reflection effect causes variations HZ Her |with Delta(m) up to 1.5m. A cycle of 34.875d duration is HZ Her |observed in X-ray band; the source is faint during HZ Her |two thirds of the cycle. The optical light curve changes HZ Her |are observed during the 35d cycle [09283]. According to HZ Her |[06539], during JD2427543 - 657 and JD2428630 - 29789 the HZ Her |strong reflection effect was absent; the star was still HZ Her |varying with P = 1.7d and had Delta(m) ~0.5m, HZ Her |Min I = Min II. In [06546] it is stated that HZ Her |such intervals with no reflection effect, of 8d to 7a HZ Her |duration, took place for almost half the time since HZ Her |1890. The light changes during such intervals are in HZ Her |the range 14.7m - 15.2m pg. Since 1957 intervals without HZ Her |the reflection effect were not observed. In June - July HZ Her |1983 the predicted phases of high X-ray flux HZ Her |did not take place, but the reflection effect did not HZ Her |disappear [09284]. Secondary light variations: P1 = HZ Her |1.0977d (delta(B1) = 0.33m), P2 = 0.871173d*E HZ Her |(delta(B2) = 0.10m), HZ Her |P3 = 1.623846d*E (delta(B3) = 0.17m) [09285]. X-ray pulsar, HZ Her |P = 1.2377991s (JD2443357), dP/dt/P = (-2.9 +- 0.2)*10**(-6)/yr HZ Her |[09286], sometimes noticeable also in the HZ Her |optical range [06543]. Rapid brightness flickering. IK Her |d = 0.030P? IQ Her |Superposition of variations with shorter P and IQ Her |small Delta(m) [06645]. IT Her |According to the spectrum, EW type is possible. KL Her |Min II 14.7. KV Her |The light curve is characteristic of Mira Ceti stars KV Her |but strongly varies. Many irregularities. O - C: -96d, +73d. LR Her |Min II 15.4:. LS Her |The light curve shape var. LT Her |d = 0.02P. Min II 10.79. LV Her |P var? During JD2428429 - 31342 - see Table. MM Her |VB A (B 13.50m, 18", 120deg). Min II 9.7. MM Her |Delta(m) of the distorsion wave up to 0.12m. MP Her |[Fe/H] = -1.18. MS Her |Min II 13.3. MT Her |Min II 12.30. MV Her |The chart in [00156] identifies the variable erroneously; MV Her |real MV Her is marked as "C". MW Her |P var. P = 503d (1976) [09290]. During MW Her |JD24668 - 29172 - see Table. MX Her |Moments of Min after JD2444000 published by different MX Her |groups of observers contradict each other. NQ Her |According to [03882], EA, 8.0 - 8.6 pg, Min II NQ Her |8.4, Min I = 2426894.433 + 0.870218d*E (JD2426894 - 34250). NR Her |Waves, P = 2.8d - 5.5d. OQ Her |Epoch of min is given. OS Her |B - V: +0.12, +0.48. OU Her |Spectral type is given according to [02198]; in BSD-G7. OX Her |Delta(S) = 6:. PW Her |Min II 10.1; DII ~0.3P(!). V0338 Her |Min II 10.13. P var. Before JD2437000 Min = V0338 Her |2433771.38 + 1.305732d*E [03115]; Min = 2441864.379 + V0338 Her |1.3057515d*E (JD2437000 - 43400) [08593,00001]; V0338 Her |since JD2443400 - see Table. V0342 Her |Min II 10.7. V0347 Her |P var. Max = 2415288.21 + 0.5373619d*E (JD2415288 - V0347 Her |18596); since JD2429495 - see Table. V0359 Her |P var. Min = 2416046.476 + 1.755754d*E (JD2416000 - V0359 Her |26500) [00001]; Min = 2435693.47 + 1.755775d*E (JD V0359 Her |2426500 - 36000) [01040]; since JD2443500 - see Table. V0362 Her |Close to DO Her. V0365 Her |Blazhko effect: Pi = 40.64d. P var. V0365 Her |During JD2429037 - 36840 - see Table. V0373 Her |P = 0.33d or 0.50d is possible. V0384 Her |P ~0.33d is possible. V0387 Her |Min II 13.2. V0394 Her |P var? V0395 Her |Z = 0.0643. V0396 Her |Z = 0.175. V0403 Her |Min II 16.0:. V0412 Her |Min II 15.2. V0422 Her |P var? During JD2434131 - 35991 - see Table. V0423 Her |Min II 15.0. V0426 Her |Min II 15.8. V0431 Her |P var. V0436 Her |The elements are uncertain. V0441 Her |IR excess, evidence for a circumstellar envelope. Possibly V0441 Her |non-radial pulsation. V0442 Her |P var. Max = 2434223.375 + 0.4421143d*E (JD2417447 - 36083); V0442 Her |since JD2435730 - see Table. V0442 Her |The shape of the light curve varies. V0446 Her |Before the outburst 16.2m - 18.8m [03607]. V0451 Her |ADS 10310 A (B 10.70m, 19", 239deg). V0451 Her |The epoch of Min U light is given. V0458 Her |[Fe/H] = -1.65. V0463 Her |P = 54.4d is possible. V0477 Her |Min II 15.4. V0482 Her |Possibly eclipsing. V0499 Her |Blazhko effect. V0502 Her |Min II 13.5? V0510 Her |P var? V0511 Her |P var? V0513 Her |Min II 15.7. V0516 Her |Min II 17.1. V0523 Her |Elements are valid during JD2430940 - 990. V0524 Her |Twice shorter P is possible. V0527 Her |Max = 2430938.451 + 0.5188d*E (JD2430938 - 990); V0527 Her |during JD2436308 - 318 - see Table. V0529 Her |Epoch of Min is given. V0529 Her |According to [04217], P = 120d. V0533 Her |VB A (B 16m, 9.5", 0deg). oscillations: V0533 Her |Max = 2443717.730281 + 0.0007364941d*E, A ~1% [04162]. V0551 Her |P = 4.00d/n is possible. V0552 Her |P = 3.04d/n is possible. V0554 Her |P = 4.01d/n is possible. V0557 Her |P = 8.00d/n is possible. V0570 Her |P = 0.5d or 0.33d is possible. V0578 Her |Red. V0582 Her |VB. Red. V0583 Her |Red. V0588 Her |Possibly eclipsing. V0600 Her |SB, Porb - see Table. Variability of Vr possibly caused by V0600 Her |BCEP type pulsations: P - 0.18d. V0601 Her |Elements are valid since JD2439184. V0604 Her |Red. V0608 Her |Blazhko effect. V0615 Her |Red. V0618 Her |P var? V0624 Her |VB A (12.04m, 40"). Min II 6.35. SB2. V0637 Her |ADS 10227 A (BC 9.2m, 9.2m, 1.7", 18deg, 1975; BC: A = V0637 Her |0.28", Porb = 56.56yr). V0639 Her |mu alpha = -0.21", mu delta = +0.39",pi = 0.087". V0639 Her |VB B (A = V647 Her, 11.36m var, dM4e; B 16", 268deg). V0639 Her |Flares in the bands U and M pg. V0640 Her |VB A (B 14.9m, 8.5", 217deg; C 13.9m, 23", 221deg). V0641 Her |L or ISB type is also possible. V0644 Her |SB (Porb = 11.859d). V0645 Her |P ~3h - 10h, a cycle of 40d. V0647 Her |VB A (B = V639 Her, 16", 268deg); mu alpha = -0.21", V0647 Her |mu delta = +0.39"; pi = 0.087". V0652 Her |P var; nonlinear term: -45.80d*10**(-10)*E**2. Delta(m) var. V0652 Her |Resembles PV TEL type stars but is a helium rich subdwarf. V0652 Her |Epoch of Max is given. Secondary hump at the phase 0.5P. V0654 Her |Delta(m) = 0.15m in white light. V0655 Her |ADS 10407 A (B 9.2m, 4.1", 144deg, 1971). V0657 Her |According to [02610], CST?, 11.0m. V0662 Her |Less probable P values: 0.56629d, 0.56710d, 0.56881d, V0662 Her |0.56970d. V0685 Her |Min II 15.8. V0687 Her |Min II 14.9. V0691 Her |Possible P values: 0.927d, 0.637d. V0697 Her |H2O, OH maser. V0699 Her |Min II 16.0:. V0717 Her |Blazhko effect? V0718 Her |Min II 14.3. V0719 Her |EW type with twice longer P is not excluded. V0720 Her |Blazhko effect? V0721 Her |Blazhko effect? V0722 Her |Min II 15.7. V0723 Her |Min II 15.5. V0728 Her |Min II 11.4. V0731 Her |Min II 13.8. V0731 Her |Twice shorter P is not excluded. V0732 Her |Min II 13.8. V0733 Her |Min II 14.3:. V0737 Her |Blazhko effect? V0740 Her |Min II 14.4. V0741 Her |Blazhko effect? V0742 Her |Min II 14.4. V0744 Her |Vr var, P = 86.7221d (SB1? nonradial pulsatiob?). V0744 Her |Rapid spectral variability is possible: P = 2.5552d, V0744 Her |0.78906d. V0749 Her |P = 465s. V0771 Her |Epoch of max U light is given. V0772 Her |VB AB (7.4m, G0V; 8.5m, G8V:; A = 0.27", E = 0.97, P = V0772 Her |20.0yr, C 10.62m, 28"). One of the components V0772 Her |(probably B) is SB1, P = 0.879511d [04056]. The same V0772 Her |component must be the eclipsing system. Faint X-ray V0772 Her |source. V0774 Her |Both flares and "antiflares" (abrupt fadings) of V0774 Her |comparable amplitude are observed. V0946 Her |Not Wolf 688, a large-proper-motion star, which is at 17h19m28s.9, V0946 Her |+33deg05'10" (epoch and equinox 2000.0). V0973 Her |Suspected rapid brightness variations. V0994 Her |The secondary component of the double system may also vary. alf Her |ADS 10418 A (B 5.39m, 4.9", 107deg, 1973; B - SB2, alf Her |G5III + F2V). Slow variations, P ~6yr, Delta(m) ~0.5m; alf Her |quicker changes, P ~ 50d - 155d, Delta(m) ~ 0.3m - 1.0m. alf Her |Together with the visual companion the alf Her |star is surrounded by an enormous envelope (R ~2*10**5R$, alf Her |expansion velocity 10 km/s, mass loss 3*10**(-8)M$/yr). nu Her |[Fe/H] = -0.26. SB? omi Her |VB interferometric. phi Her |SB, Porb = 560.5d. ome Her |ADS 10054 A (B 11.5m, 0.8", 232deg, 1967; C 11.0m, 28.4", ome Her |96deg, 1957; D 27.5", 271deg, 1960). Epoch of Min is given. ome Her |Double wave in the light curve. ome Her |Rapid variations, P = 0.15d [09310]. g Her |The mean cycle 1972 - 1981 is given. Slow pulsations g Her |(<P> = 875d +- 70d) and non-periodic variations on the g Her |time scale of 5d - 15d with Delta(m) up to 0.2m are g Her |superimposed. u Her |ADS 10449 A (B 10.2m, 4.4", 60deg). Min II 4.93. R Hor |OH, H2O, SiO maser. P var. Max = 2428868 + 401.5d*E R Hor |(JD2412800 - 28900); since JD2428900 - see Table. V Hor |<P> = 59d (JD2428380 - 910), <P> = 90d (JD2429170 - 980). X Hor |Epoch of Min brightness is given. Maxima are broad. X Hor |Usually secondary minima are observed. SY Hor |Min II 12.0. SZ Hor |Min II 10.7:. TU Hor |Min II 6.03; Min II - Min I = 0.52P; TU Hor |Max II is fainter than Max I by 0.05m. Peculiar TU Hor |ellipsoidal variable [09245]. TY Hor |Type RCB? UU Hor |P var. Max = 2416826.417 + 0.6436900d*E (JD2416800 - 25000); UU Hor |since JD2425000 - see Table. UX Hor |Min II 14.4. P var. Min I = 2426659.380 + 0.7126943d*E UX Hor |(JD2426650 - 30860); since JD2430540 - see Table. UZ Hor |P var. Max = 2426679.425 + 0.338188d*E (JD2426300 - 28430); UZ Hor |since JD2430040 - see Table. VY Hor |mu = 0.173", ro = 33deg. P = 314s, 617s. R Hya |VB A (B 13.0m, 21.6", 324deg). SiO maser. P var. According R Hya |to [00458]; Max = 2328201 + 486d*E (JD2328200 - 31120); R Hya |Max = 2343512 + 507d*E (JD2343300 - 44800); R Hya |Max = 2372678 + 485d*E (JD2372200 - 72700); R Hya |Max = 2380447 + 477d*E (JD2380000 - 81400); R Hya |Max = 2385160 + 461d*E (JD2384700 - 88000); R Hya |Max = 2394350 + 448.6d*E (JD2393900 - 2402000); R Hya |Max = 2403742 + 434d*E (JD2403300 - 04200); R Hya |Max = 2406363 + 429.5d*E (JD2406000 - 11100); R Hya |Max = 2413642 + 411d*E (JD2413200 - 14100); R Hya |Max = 2416563 + 405.5d*E (JD2416100 - 23400); R Hya |Max = 2424288 + 414.7d*E (JD2423400 - 28500). R Hya |since JD2428500 - see Table. T Hya |P var. Max = 2399455 + 289.00d*E(JD2398600 - 2421700); T Hya |Max = 2422584 + 294.2d*E (JD2421700 - 25800); T Hya |Max = 2431781 + 284.20d*E (JD2425800 - 36200); since T Hya |JD2437500 - see Table. V Hya |VB A (B 11.58mV, KO III, 46", 186deg). V Hya |Mean brightness variations with P = 6670d and A = 3.5m are V Hya |superimposed by light oscillations with A = 1.1m - 2m and V Hya |elements given in the Table. Deep light minima were V Hya |observed in 1891, 1908, 1925, 1942 - 43, 1959, and 1962. V Hya |A graph of the light curve [03614]. W Hya |VB A (B 9.3m, 72", 108deg). P var. Max = 2411074 + 379d*E W Hya |(JD2411000 - 14150); Max = 2414644 + 395d*E W Hya |(JD2414150 - 19400); Max = 2419746 + 378d*E W Hya |(JD2419400 - 25200) [00458]. Max = 2425740 + 366d*E W Hya |(JD2425200 - 27000); Max = 2440336 + 397.35d*E W Hya |(JD2428000 - 40500); since JD2440500 - see Table. W Hya |Amplitude and shape of the light curve vary strongly. W Hya |OH, H2O, SiO maser. X Hya |OH, H2O, SiO maser. Y Hya |Mean magnitude varies. RR Hya |H2O maser. RS Hya |P var. Max = 2422973 + 330.2d*E (JD2414000 - 23000); RS Hya |Max = 2429126 + 342.0d*E (JD2423000 - 29200); Max = RS Hya |2429455 + 331.2d*E (JD2429200 - 34500); RS Hya |since JD2434500 - see Table. RT Hya |Before 1952 <P> = 255d; since 1952 - see Table. RT Hya |The character And amplitude of light variations vary RT Hya |strongly. RU Hya |OH, H2O maser. P var. Max = 2429572 + RU Hya |334.0d*E (JD2414000 - 29600); since JD2428500 - see RU Hya |Table. RW Hya |SB2 (P = 370d). Epoch of Min brightness is given. RX Hya |VB A (B 10.5m). Depth of Min II 0.05m. P var. RX Hya |Min I = 2428261.385 + 2.2815942d*E (JD2419500 - RX Hya |28500); Min I = 2440650.409 + 2.2816200d*E RX Hya |(JD2428500 - 41400); since JD2441400 - see Table. SS Hya |VB A (B 12.0m, 13", 195deg); SB2. SU Hya |Mean magnitude varies with P = 780d. SV Hya |VB A (B 35", 225deg). Delta(S) = 7. SX Hya |D = 0.022P. P var. Min I = 2427659.223 + 2.895697d*E SX Hya |(JD2410000 - 28000) [00007]; since JD2442500 - see Table. SY Hya |P var. Min = 2425590.589 + 3.403082d*E (JD2425500 - SY Hya |31150) [07548]. Since JD2432200 - see Table. SZ Hya |P var. Max = 2415714.1429 + 0.53742815d*E SZ Hya |(JD2414700 - 26500) [03626]; Max = 2426410.575 + 0.53736d*E SZ Hya |(JD2426400 - 27200) [00001]; Max = 2431881.5537 + SZ Hya |0.53723051d*E (JD2427880 - 35200) [03626]; Max = SZ Hya |2435542.267 + 0.5372497d*E (JD2435500 - 38900) SZ Hya |[03627]. Since JD2438770 - see Table. SZ Hya |Blazhko effect: Max(A) = 2440705 + 25.8d*n [06557]; SZ Hya |10.44m <= Max <= 11.03m. TT Hya |Min II 7.32; d = 0.035P. TU Hya |P var. Max = 2416980 + 277.5d*E (JD2412500 - TU Hya |17300); Max = 2417260 + 272.5d*E (JD2417200 - TU Hya |19800) [01787]; Max = 2430410 + 281.4d*E TU Hya |(JD2420500 - 30500); Max = 2438332 + 272.3d*E TU Hya |(JD2432000 - 39200); since JD2439200 - see Table. TY Hya |P var. Min = 2434478.464 + 4.660978d*E (JD2419800 - TY Hya |35000) [01788]; since JD2435000 - see Table. UU Hya |P var. Max = 2427423.84 + 0.5238585d*E (JD2414950 - 27400) UU Hya |[01789]; Max = 2429729.835 + 0.523854d*E (JD2427000 - 31000) UU Hya |[00752]. Spectrum is based on Ca II. UW Hya |Min II 13.8:; Min II - Min I = 0.64P. P = 1.055439d? UY Hya |Min II 13.8. RRC? VV Hya |P var. Max = 2427421 + 155d*E (JD2419500 - 37000) VV Hya |[01792]; since JD2437000 - see Table. VX Hya |(k - b)2 = 0.26. VX Hya |Luminosity class [03149] contradicts the type of light VX Hya |variability. The shape of the light curve strongly varies. VX Hya |The main oscillation with the period P0 given in the Table VX Hya |is superimposed by the secondary one with P1 = 0.172720d VX Hya |[03631]. P1/P0 = 0.773; Pb = 0.761445d. VY Hya |Min II 9.1. VZ Hya |Min II 9.46. WY Hya |Min II 11.2. WZ Hya |(k - b)2 = 0.06. P var. Max = 2416169.681 + 0.53772640d*E WZ Hya |(JD2414000 - 19000); Max = 2419811.736 + WZ Hya | + 0.53775858d*E (JD2419000 - 21000); Max = WZ Hya | = 2424618.630 + 0.53774101d*E (JD2421000 - 32000) WZ Hya |[00752]; Max = 2436613.445 + 0.5377229d*E WZ Hya |(JD2436600 - 38500) [03633]; since JD2438000 - see Table. XX Hya |P var. Max = 2439560.355 + 0.50774868d*E XX Hya |(JD2428200 - 39560) [05238]; since JD2439560 - see Table. XZ Hya |Min II 15.0. AE Hya |Min II 14.6. AF Hya |Min II 13.8. AI Hya |Min II 9.84; Min II - Min I = 0.438P; DII = 0.075P; AI Hya |dI = 0.02P; dII = 0.00P; EA/DM. Pulsation AI Hya |period P' = 0.13803d, A = 0.02m - 0.03m [09259]. AV Hya |Min II 10.35; dI = 0.023P:. CH Hya |Min II 15.5; Min II - Min I = 0.57P. CO Hya |Found in Lupus, in 10deg to the south from the position CO Hya |published by the discoverer [00078]. CW Hya |P var? [04027]. CW Hya |Elements given in the Table satisfy observations only in CW Hya |the interval JD2428950 - 30375. DD Hya |P var. Max = 2431139.313 + 0.501818d*E (JD2431100 - DD Hya |600) [01432]. Since JD2441600 - see Table. DE Hya |d = 0.014P? DF Hya |Min II 11.5. DH Hya |Delta(S) = 7. DK Hya |Min II 10.7. DM Hya |d = 0.15P? EU Hya |Min II 10.2. EX Hya |Light variations with Porb and amplitude up to 0.9mV EX Hya |due to eclipses of hot spot are represented by the EX Hya |elements: ET(Min) = 2437699.94177 + 0.0682338422d*E, EX Hya |where ET(Min) is the heliocentric Julian Date converted EX Hya |to Ephemeris Time; simultaneously periodic modulation of EX Hya |the shape of the light curve between the outbursts is EX Hya |observed with the amplitude 0.2m - 0.9m and the elements: EX Hya |Max = 2437699.8895 + 0.04654656d*E - 1.2d*10**(-12)*E**2 EX Hya |[09265]. Mean interval between bright outbursts is 465d EX Hya |[05695], mean cycle is close to 20 - 30d. EY Hya |P var. Max = 2432707 + 160.5d*E (JD2426100 - 32800); EY Hya |since JD2432800 - see Table. EZ Hya |Min II 10.7. P var. Min I = 2440255.8482 + 0.44976658d*E EZ Hya |(JD2431160 - 40650) [07549]; since JD2440250 - see Table. FG Hya |Min II 10.25; dI = dII = 0.085P. P var. Min I = FG Hya |2431150.388 + 0.3278422d*E (JD2431140 - 34400) FG Hya |[00182]; Min I = 2436968.7067 + 0.32783433d*E FG Hya |(JD2434050 - 400) [03639]; Min I = 2436968.7067 + FG Hya |0.32783546d*E (JD2436950 - 43250) [09267]; FG Hya |since JD2444600 - see Table. FI Hya |V27 in the globular cluster NGC 4590 FI Hya |(M68); cluster non-member. FS Hya |According to [01480] P = 91.7d. FW Hya |Min II 12.4. FY Hya |VB A (B 15.45m, 15", 90deg); Delta(S) = 7:; (k - b)2 = -0.03. GK Hya |Min II 9.57. GK Hya |There is a square term in the elements: GK Hya |-4.01d*10**(-9)*E**2. GM Hya |d <= 0.01P. GN Hya |Min II 13.6. GT Hya |Cep? HS Hya |Min II 8.55. IK Hya |Blazhko effect with Pi ~30d. IW Hya |OH, H2O maser. KM Hya |P var? KU Hya |VB AB (7.3m, 7.4m, A = 0.150", P = 58.93 yr, E = 0.219); KU Hya |A(v) = 0.06m. KW Hya |Porb = 7.75043d; E = 0.110 [09273]; Min II 6.35; KW Hya |Min II - Min I = 0.54P. bet Hya |VB A (B 5.6m, 0.9", 8deg, 1959). khi 2 Hya |Min II 5.92. Y Hyi |d = 0.024P. RR Hyi |In the constellation Octans. RS Hyi |In the region of the Small Magellanic Cloud. RS Hyi |Not a member of the cloud. RT Hyi |Min II 14.1. RV Hyi |Min II 12.4; Min II - Min I = 0.61P. RY Hyi |In the region of the Small Magellanic Cloud. Not a member RY Hyi |of the Cloud. ST Hyi |The member of the Small Magellanic Cloud. [A/H] = -0.8. SZ Hyi |In the region of the Small Magellanic Cloud. Not a member SZ Hyi |of the Cloud. TW Hyi |Delta(S) = 10:. UU Hyi |P = 112.25d? VW Hyi |Mean interval between the supermaxima is 179d. VW Hyi |Porb = 0.0742711d. Between the normal outbursts the VW Hyi |brightness periodically increases by 0.35m - 0.40m because VW Hyi |of hot spot appearances: VW Hyi |Max = 2440128.0222 + 0.0742711d*E [07550]. During the VW Hyi |supermaxima the period between the superhumps is VW Hyi |0.0769d [09275]. Sometimes the light oscillations with VW Hyi |the amplitude 2% and cycle from 28s to 34s are observed VW Hyi |[07551]. VY Hyi |In the region of the Small Magellanic Cloud. Not a member VY Hyi |of the Cloud. VZ Hyi |RR [00193]. WX Hyi |Mean interval between the supermaxima is 141.5d. WX Hyi |Porb = 0.0748134d [09277]. Period between the superhumps WX Hyi |observed during the supermaxima is 0.07737d [09278]. WZ Hyi |In the region of the Small Magellanic Cloud. Not a member WZ Hyi |of the Cloud. ZZ Hyi |A galaxy PGC 232232 [00001]. AC Hyi |In the region of the Small Magellanic Cloud. Not a member AC Hyi |of the Cloud. BB Hyi |Delta(S) = 7:. V Ind |P var. Max = 2439792.276 + 0.4796030d*E V Ind |(JD2414000 - 40000) [05233]; since JD2440000 - see Table. V Ind |Delta(S) = 7, (k - b)2 = 0.02. RS Ind |Min II 10.0. P var. RU Ind |VB A (B 12.6m, 2.3", 103deg). Min II 12.1. RX Ind |240d < P < 310d. RY Ind |Min II 11.04. ST Ind |Min II 11.79. SU Ind |Min II 9.5:. TV Ind |Min II 11.9. AR Ind |Min II 14.4. RRC? AY Ind |mu alpha = +0.345", mu delta = -0.310"; VB? R Lac |VB A (B 14.1m, 6", 50deg). S Lac |P var. Max = 2412857 + 238.2d*E (JD2410000 - 16400); S Lac |Max = 2418828 + 241.45d*E (JD2416400 - 20500); Max = S Lac |2427307 + 242.7d*E (JD2420500 - 27300); Max = S Lac |2437290 + 237.4d*E (JD2427300 - 37300); S Lac |since JD2437300 - see Table. U Lac |There are light variations with the periods: U Lac |150d, 550 - 690d, 2900d. V Lac |P var. There is a square term in the elements: V Lac |-6.48d*10**(-8)*E**2. W Lac |P var. Max = 2415255 + 323d*E (JD2414600 - 15300); W Lac |Max = 2425628 + 335.5d*E (JD2425600 - 38000) [00458]; W Lac |Max = 2433844 + 324.5d*E (JD2428000 - 33850); W Lac |since JD2433850 - see Table. X Lac |P var. Max = 2418890.497 + 5.444303d*E (JD2416670 - X Lac |29500) [02033]; since JD2429500 - see Table. Z Lac |P var. There is a square term in the elements: Z Lac |-3.4d*10**(-8)*E**2. [A/H] = 0.2. RR Lac |P var. Max = 2419434.331 + 6.416146d*E (JD2417900 - 31600); RR Lac |since JD2431600 - see Table. [A/H] = 0.0. RT Lac |Min II 9.62. P var. Min I = 2440382.9005 + 5.0740484d*E + RT Lac |1.02d*10**(-8)*E**2 (JD2411650 - 42500) [08592]; RT Lac |since JD2436470 - see Table. RT Lac |There is a square term in the elements given in the Table: RT Lac |-2.7d*10**(-8)*E**2. Shape of the light RT Lac |curve and depths of the Minima vary. According to RT Lac |[09293] the period of the distortion wave migration is RT Lac |~9.5 yr, the period of the wave amplitude variations RT Lac |(0 < A <= 0.17m) is ~30 yr. According to [09292] the RT Lac |migration period is nearly half of the value given in RT Lac |[09293]. RV Lac |Mean magnitude varies with the period 550 - 700d. RW Lac |Min II 10.8; DII = 0.024P; Min II - Min I = 0.492P. RX Lac |S7.5/1e. P = 174d (JD2414950 - 29550) [01026]; RX Lac |since JD2436800 - see Table. RY Lac |Oscillations of mean magnitude with P = 300 - 420d RY Lac |and A <= 0.5m are superimposed by oscillations with RY Lac |P = 38 - 91d. SS Lac |Probable member of the open cluster NGC 7209. Min II 10.5; SS Lac |Min II - Min I = 0.57P; d = 0.008P. SS Lac |Apsidal motion with P = 1000 yr is possible. ST Lac |Elements should be checked. SU Lac |P var. Max = 2412748 + 279.10d*E (JD2412700 - 27000) SU Lac |[05707]; Max = 2426972 + 286.74d*E (JD2426900 - 31000); SU Lac |Max = 2431008 + 306.0d*E (JD2431000 - 33150) SU Lac |[00001]; Max = 2433150 + 319.14d*E (JD2433150 - 42150) SU Lac |[05707]; since JD2442100 - see Table. SW Lac |Min II 9.31. P var. Min I = 2418943.712 + 0.32071236d*E SW Lac |(JD2410000 - 19990); Min I = 2420038.621 + SW Lac |0.32071510d*E (JD2419990 - 25210); Min I = SW Lac |2430996.525 + 0.32071665d*E (JD2425210 - 33690); SW Lac |Min I = 2436046.5634 + 0.32072132d*E (JD2433690 - 36755) SW Lac |[05222]; Min I = 2437572.5723 + 0.32072811d*E SW Lac |(JD2436755 - 40000) [03374]; Min I = 2440467.4592 + SW Lac |0.32072480d*E (JD2440110 - 40500) [06089]; Min I = SW Lac |2441249.3737 + 0.3207197d*E (JD2440500 - 41600); SW Lac |[00001]; Min I = 2442697.4039 + 0.3207144d*E SW Lac |(JD2441600 - 43100) [09295]; Min I = 2443459.7476 + SW Lac |0.3207216d*E (JD2443100 - 44400) [09297]; Min I = SW Lac |2444856.8064 + 0.3207184d*E (JD2444400 - 44900) SW Lac |[00001]; since JD2444900 - see Table. SW Lac |Shape of the light curve, depths of minima and heights SW Lac |of maxima vary. TW Lac |d = 0.018P. P var. Min I = 2424387.332 + 3.0374936d*E TW Lac |(JD2424380 - 34000) [02389]; Min I = 2434049.593 + TW Lac |3.037520d*E (JD2434000 - 36560) [03115]; TW Lac |since JD2441500 - see Table. TZ Lac |In the region of the open cluster NGC 7243. UW Lac |Depth of Min II 0.05m; d = 0.028P. P var. UW Lac |Min I = 2429158.17 + 5.2902d*E (JD2414580 - 29440) UW Lac |[01813]; Min I = 2429158.17 + 5.290000d*E UW Lac |(JD2429440 - 35800) [03115]; since JD2436800 - see Table. UW Lac |Apsidal motion is possible [09300]. UY Lac |d = 0.022P. UZ Lac |P var? VX Lac |P var. Min = 2424791.488 + 1.0744891d*E VX Lac |(JD2424700 - 32400); Min = 2432479.477 + 1.0744991d*E VX Lac |(JD2432400 - 40510); Min = 2440750.971 + VX Lac |1.0744881d*E (JD2440750 - 43000) [07552]; VX Lac |since JD2443000 - see Table. VY Lac |Min II 10.6. P var? Min I = 2434629.392 + 1.036245d*E VY Lac |(JD2424700 - 39830) [01804]; since JD2440080 - see Table. WY Lac |Light variations with P = 850d and A = 1.5m are WY Lac |superimposed by variations with P = 50d and A = 1m. XX Lac |In the region of the open cluster NGC 7243. XZ Lac |P var. AG Lac |Min II 14.0. AR Lac |Min II 6.43; Min II - Min I = 0.5018P; dI = 0.045P; DII = AR Lac |0.13P; dII = 0.00P. P var. Min I = 2426624.378 + AR Lac |1.983244d*E (JD2415300 - 26800) [09309]; Min I = AR Lac |2429535.739 + 1.9832125d*E (JD2426800 - 36000) AR Lac |[09312]; Min I = 2437018.414 + 1.983252d*E AR Lac |(JD2436000 - 37500) [00001]; since JD2437500 - see Table. AR Lac |There is a square term in the elements AR Lac |given in the Table: - 5.24d*10**(-9)*E**2. AR Lac |Shape of the light curve varies; there is a AR Lac |distortion wave with A up to 0.13mV migrating in the AR Lac |direction of decreasing phases with P ~2.5 yr. Spectrum AR Lac |investigations [01816,09315,9316]. AU Lac |Min II 12.2; Min II - Min I = 0.53P. AW Lac |Min II 11.2. BH Lac |Hydrogen lines in the spectrum are sharp and deep [03149]. BL Lac |Z = 0.07; <B-V> = +1.0. Light curve graph [06784]. BM Lac |The elements are valid in the interval JD2425200 - 26250. BT Lac |There is a square term in the elements: -0.0004d*E**2. BT Lac |Epoch of Max brightness is given in the Table. BT Lac |Mean brightness varies in the range 13.8m - 15.2m with BT Lac |P = 654d. Mean amplitude of the shortperiodical variations BT Lac |is ~1.5m. There occur changes of primaries and BT Lac |secondaries minima into each other. BU Lac |The main variation is superimposed by waves with a BU Lac |possible period -200d. CG Lac |Min II 14.0. CM Lac |Min II 8.53; DII = 0.12P. CN Lac |Min II 12.6. In the region of the CN Lac |open cluster NGC 7209. Not member of the cluster. CO Lac |Min II 10.79. Apsidal motion with CO Lac |P = 42.3 yr is observed. There is a periodic term in CO Lac |The elements given in the Table: -0.0133d cos(157.7deg + CO Lac |0.0359deg*E). Min II = 2427534.8439 + 1.5422075d*E + CO Lac |0.0133d cos(157.7deg + 0.0359deg*E). CS Lac |Min II 9.4. CZ Lac |Delta(S) = 1. P var. Max = 2432878.234 + 0.43210346d*E CZ Lac |(JD2428700 - 39400) [01442]; Max = 2443081.309 + CZ Lac |0.4319850d*E (JD2439400 - 43100) [05839]; Max = CZ Lac |2444080.122 + 0.432114d*E (JD2443800 - 44100) CZ Lac |[09009]; since JD2445100 - see Table. DD Lac |VB A (B 9.2m, 69", 16deg). P var. Max = 2421914.178 + DD Lac |0.19309018d*E - 0.001798d*10**(-8)*E**2 (JD2421400 - DD Lac |37600) [05711]; since JD2443000 - see Table. DD Lac |According to [09337] simultaneously the pulsations with DD Lac |the following periods are observed (the corresponding AB DD Lac |values are given in the brackets): P1 = 0.193082d (0.080m), DD Lac |P2 = 0.197382d (0.034m), P3 = 0.182115d (0.020m), DD Lac |P4 = 0.187438d (0.016m), P5 = 0.095109d (0.010m), DD Lac |P6 = 0.23583d (0.008m). A var; 0.04m <= A <= 0.12m. DE Lac |Delta(S) = 5. P var. Max = 2428807.130 + 0.2536940d*E DE Lac |(JD2427000 - 33000); Max = 2433005.766 + 0.2536929d*E DE Lac |(JD2433000 - 39100) [03378]; since JD2442000 - see Table. DF Lac |[A/H] = 0.2. DG Lac |P var. Min = 2426266.355 + 2.206435d*E (JD2426200 - 40000) DG Lac |[04961]; since JD2440000 - see Table. DH Lac |P var. Max = 2418240 + 284.8d*E (JD2418000 - 27350); DH Lac |since JD2427300 - see Table. DM Lac |Erroneously labeled VV306, instead of VV307, in the chart [05862]. DO Lac |According to [00085], EA. EG Lac |P > 50d? [05386]. EM Lac |Min II 13.09. EN Lac |VB A (B 11.32mV, 27", 345deg; C 9.0mV, 62", 48deg); SB1 EN Lac |(Porb = 12.0968d). Eclipsing system with a pulsating EN Lac |primary component of BCEP type. Depth of Min I 0.05mB. EN Lac |Min I = 2444909.4339 + 12.096816d*E; D = 0.015P, EN Lac |d = 0.000P. Simultaneously pulsations are EN Lac |observed with the periods P1 = 0.169170d, P2 = 0.170770d, EN Lac |P3 = 0.181692d [09346]. The corresponding amplitudes EN Lac |of pulsations vary. The values of the amplitudes in EN Lac |B system are as follows: A1 = 0.046m, A2 = 0.024m, EN Lac |A3 = 0.022m (1952 - 1965); A1 = 0.016m, A2 = 0.010m, EN Lac |A3 = 0.014m (1977); A1 = 0.010m, A2 = 0.014m, A3 = 0.023m EN Lac |(1980 - 81). 0.01m <= A <= 0.11m. EO Lac |Min II 12.9; Min II - Min I = 0.485P. EP Lac |Depth of Min II 0.04m. ER Lac |Depth of Min II 0.05m:. ES Lac |Min II 11.6; Min II - Min I = 0.57P. ES Lac |Apsidal motion is possible: ES Lac |Min II = 2433582.95 + 4.459451d*E [09347]. EU Lac |The chart in [05862] is wrong. EV Lac |VB A (B 12.74mB, 10", 260deg, 1949); mu alpha = -0.065s, EV Lac |mu delta = -0.46". Dark companion (A = 0.0206", P = 45 yr, EV Lac |E = 0.5) [09348]. In 1979 sinusoidal light oscillations EV Lac |were observed in the range 10.20m - 10.27mV: EV Lac |Min = 2444037.576 + 4.378d*E [09349]. In 1974 - 76 such EV Lac |periodicity was not observed [09350]. EW Lac |Non-radial pulsations with P = 0.7d - 0.8d EW Lac |are also possible [09351,09352]. EX Lac |d = 0.050P. FQ Lac |A var; P var. Elements given in the Table are valid in the FQ Lac |intervale JD2427950 - 31700. FU Lac |d = 0.013P. GS Lac |Min II 15.2. GX Lac |Min II 10.23. HK Lac |SB1 (Porb = 24.4284d [09355]). HM Lac |Depth of Min II 0.05m. HN Lac |Min II 14.7. HQ Lac |Erroneously labeled VV307, instead of VV306, in the chart [05862]. HR Lac |Min II 14.3. HT Lac |In the region of the open cluster NGC 7209. HW Lac |Min II 14.8. HX Lac |Min II 14.8. HZ Lac |Min II 15.0. IM Lac |Min II 13.2. IN Lac |E? IP Lac |Min II 14.0. IR Lac |Min II 15.4; d = 0.03P. IT Lac |P var. IU Lac |Min II 13.5. IY Lac |Blazhko effect? IZ Lac |Min II 12.7. KO Lac |Min II 14.7. KP Lac |P < 1d. KR Lac |Min II 15.8; dII = 0.05P. KS Lac |Depth of Min II 0.03m. KU Lac |Depth of Min II 0.03m. LU Lac |Min II 15.32. LW Lac |d = 0.03P. Depth of Min II 0.03m? LY Lac |Min II 12.6. LZ Lac |Min II 12.5. MO Lac |d = 0.04P. Depth of Min II 0.05m. MP Lac |Min II 12.5. MV Lac |Min II 15.0. MZ Lac |Min II 12.1; Min II - Min I = 0.713P. MZ Lac |Min II = 2433872.702 + 3.158719d*E. Elements for Min I MZ Lac |are given in the Table. NN Lac |d = 0.02P. np (usually brighter) component of a close pair. NN Lac |The range of combined brightness is given in the Table. NO Lac |Depth of Min II 0.03m. NR Lac |Min II 13.4. Sp (brighter) component of a close pair. The NR Lac |range of combined brightness is given in the Table. NU Lac |EW? NW Lac |Min II 13.9. Close binary, the components of which are NW Lac |equal in brightness at minimum light. The range of NW Lac |combined brightness is given in the Table. OO Lac |Min II 12.8. OV Lac |150d <= P <= 200d. OX Lac |Depth of Min II 0.04m. PP Lac |Min II 12.0. PT Lac |Min II 15.4. PZ Lac |In the region of the open cluster NGC 7243. QQ Lac |In the region of the open cluster NGC 7243. QU Lac |Depth of Min II 0.04m. V0335 Lac |Min II 15.8. V0338 Lac |In the region of the open cluster IC 1434. V0339 Lac |P = 3.4084964d? V0340 Lac |Min II 12.4; Min II - Min I = 0.762P; V0340 Lac |Min II = 2432858.521 + 19.943102d*E. V0340 Lac |Elements for Min I are given in the Table. V0342 Lac |Min II 12.9. V0343 Lac |Min II - Min I = 0.57P. Depth of Min II 0.03m:. V0344 Lac |Min II 13.0. Min I = 2433873.5784 + 0.39222768d*E V0344 Lac |(JD2432800 - 35800); since JD2445200 - see Table. V0345 Lac |Min II 11.6; Min II - Min I = 0.340P; DII = 0.040P; V0345 Lac |dII = 0.014P. Apsidal motion is possible. V0347 Lac |VB. V0350 Lac |VB A (B 9.7m, 66", 94deg); SB1 (P = 17.755d [09356]). V0350 Lac |Min II 6.45 [07468]. Mean magnitude varies. See also [08933]. V0355 Lac |Northern component of a pair. V0360 Lac |SB2 (P = 10d [09357]). Min II 5.93. V0362 Lac |VB A (B 13.2m, 1.8", 49deg). V0363 Lac |VB A (B 11.3m, F6 III - V:, 6.3", 325deg). V0364 Lac |Min II 9.15; Min II - Min I = 0.52P; dI = 0.003P, V0364 Lac |DII = 0.077P, dII = 0.009P. V0412 Lac |SB, Porb = 41.95yr. V0413 Lac |SB, Porb = 2.9833d. V0442 Lac |Quasi-periodic brightness variations of a planetary nebula, possibly V0442 Lac |due to variable mass loss or pulsations. R Leo |P var. Max = 2385112 + 312.43d*E (JD2385100 - 2402500); R Leo |Max = 2402929 + 314.33d*E (JD2402500 - 11500); R Leo |Max = 2411416 + 308.93d*E (JD2411500 - 16500); R Leo |Max = 2416984 + 317.84d*E (JD2416500 - 22500); R Leo |Max = 2423328 + 312.75d*E (JD2422500 - 27000); R Leo |Max = 2427081 + 307.40d*E (JD2427000 - 30000); R Leo |Max = 2437337 + 312.13d*E (JD2430000 - 37500); R Leo |since JD2437500 - see Table. SiO, H2O, OH maser. S Leo |P var. Max = 2420654 + 189.24d*E (JD2420200 - 26100); S Leo |Max = 2426142 + 185.92d*E (JD2426100 - 28100); S Leo |since JD2428100 - see Table. T Leo |SB1 (Porb = 0.05881873d [09304]). V Leo |H2O maser. W Leo |P var. Max = 2434651 + 385.41d*E (JD2409500 - 35000); W Leo |since JD2437500 - see Table. OH maser. Y Leo |P var. Min = 2422372.520 + 1.6860978d*E (JD2418000 - 23500) Y Leo |[02389]; Min = 2422372.5368 + 1.68607314d*E Y Leo |(JD2423500 - 38600) [09307]; since JD2438600 - see Table. Y Leo |There is periodic term in the elements given in the Table: Y Leo |+0.00375d*sin(0.21487deg*E + 141.7deg). Depth of Min II Y Leo |0.1m IR. RR Leo |Delta(S) = 7.1. P var. Max = 2430440.3385 + 0.45238172d*E + RR Leo |1.963d*10**(-10)*E**2 (1898 - 1977) [08299]; since RR Leo |JD2441400 - see Table. RT Leo |Min II 10.5. RW Leo |P var. Before JD2440800 Min = 2424993.458 + RW Leo |1.6825365d*E [03115]; since JD2440800 - see Table. RX Leo |Delta(S) = 6.8. SS Leo |P var. Max = 2415485.723 + 0.62633242d*E SS Leo |(JD2414000 - 22000) [00752]; since JD2422000 - see Table. SS Leo |[Fe/H] = -1.59. ST Leo |(k - b)2 = 0.08. SZ Leo |P var. Before JD2442500 Max = 2425331.400 + SZ Leo |0.5340833d*E [04157]; since JD2442500 - see Table. SZ Leo |Light curve shape var? TV Leo |P var. Max = 2419852.318 + 0.6728362d*E TV Leo |(JD2419000 - 28000) [00001]; since JD2437000 - see Table. TV Leo |(k - b)2 = -0.01. TX Leo |VB A (B 7.8m, 2", 157deg, 1971); TX Leo |A binary according to lunar occultation data: ro = 0.0005". TX Leo |The range of combined brightness is given. TX Leo |Min II 5.69; DII = 0.19P; Min II - Min I = 0.550P. TY Leo |Elements need confirmation. TU Leo |Minor planet (8) Flora. UU Leo |Min II 11.5. P var. Since JD2430000 - see Table. UV Leo |Min II 9.49; d = 0P014. P var. Before JD2434000 UV Leo |Min I = 2425574.302 + 0.60008516d*E [07554]; UV Leo |since JD2434000 - see Table. UX Leo |Min II 10.4. UX Leo |Moments of Min by BBSAG contradict the tabulated elements. UZ Leo |Min II 10.12. P var, nonlinear term: +2.8d*10**(-12)*E**2. XX Leo |Min II 11.4. Period should be checked. XY Leo |Min II 9.80. P var. Min = 2435195.66306 + 0.2841091d*E XY Leo |(JD2434000 - 36500) [03392]; Min = 2437376.465 + XY Leo |0.28409592d*E (JD2436500 - 40000) [00001]; Min = XY Leo |2441005.5364 + 0.28410727d*E (JD2441000 - 44000) XY Leo |[09084]; since JD2444000 - see Table. XY Leo |The light curve shape var. XZ Leo |Min II 11.1. AB Leo |Epoch of Min is given. AB Leo |According to [01853], Max = 2428880 + AB Leo |103.2d*E (JD2414600 - 19000, 2428000 - 31600); AB Leo |During other time intervals cycles 75d - 125d. AD Leo |mu = 0.49", P = 265deg; pi = 0.20". AD Leo |X-ray and radio source. Astrometric binary? AF Leo |H2O maser. AM Leo |VB A (B 10.64m, 11", 270deg). Min II 9.83. AP Leo |Min II 9.88. P var. Min = 2414986.868 + 0.430350d*E AP Leo |(JD2414700 - 18600); since JD2418600 - see Table. AP Leo |Light curve shape var. AQ Leo |Elements for fundamental mode pulsations (P0) see Table. AQ Leo |For the first overtone: P1 var?; AQ Leo |P1 = 0.4101369d (1929 - 1969); P1 = 0.410130d (1957 - AQ Leo |1969); during 1973 - 1975 Max1 = AQ Leo |2441766.486 + 0.4101487d*E. delta(M0) = 0.23m, AQ Leo |delta(M1) = 0.46M. AU Leo |Vr = +7545 km/s. Variability is doubtful. BB Leo |[Fe/H] = -1.32. BL Leo |Min II14.4. P var. Since JD2442000 - see Table. BV Leo |Min II 16.1. BW Leo |Min II 15.4. BX Leo |[Fe/H] = -1.23. BZ Leo |Min II 15.8. CD Leo |Light curve shape var. CE Leo |Min II 12.5. P var? CE Leo |Min by BBSAG contradict the tabulated elements. CN Leo |Mu = 4.7", P = 235deg; pi = 0.41". CN Leo |Soft X-ray source, radio source. CW Leo |Dust envelope, 6"*4". CW Leo |Molecular radioemission: SiO, SiS, HCN, HC3N, CO, H2O, CW Leo |NH3, etc. Polarization in I band up to 24%. CX Leo |VB A (B 12.3m, 132deg); SB (Porb = 12685.4d). CY Leo |mu = 0.307", P = 141.3deg; pi = 0.022". CY Leo |Outside flares Delta(m) < = 0.036m; P = 600s, 822s, 1638s CY Leo |[06209]. A single strong flare with delta(M) = 0.61m in CY Leo |blue light of 10 Min duration was observed [06141], CY Leo |which is attributed by several authors to the presence of CY Leo |a red flaring companion. DE Leo |P = 1.2d - 2.0d? DG Leo |VB B (A 6.6m, A 8IV, SB2, Porb = 4.15d; B 6.9m, 0.271", DG Leo |211.2deg, 1980, Porb ~200yr). DG Leo |The range of the bombined brightness is given. DH Leo |SB1, Porb = 1.070354d. DK Leo |mu alpha = -0.097", mu delta = -0.214". FL Leo |Variability range according to E.M. Halbedel, IBVS No. 3502, 1990. FX Leo |Not a nearby star (despite having a Gl number). R LMi |SiO, H2O, OH mazer. T LMi |Min II 10.97. P var. Min I = 2420573.698 + 3.019889d*E T LMi |(JD2420200 - 25000); Min I = 2423856.323 + T LMi |3.0199336d*E (JD2423800 - 35500); since JD2438400 - see T LMi |Table. U LMi |1m <= A <= 3.3m. Periodicity sometimes breaks down. V LMi |Delta(S) = 5.7. Y LMi |P var. Max = 2428636.322 + 0.52443938d*E + 0.0597d* Y LMi |*sin(0.0657deg*E + 27.2deg) (JD2425250 - 28500); Max = Y LMi |2428636.348 + 0.5244564d*E (JD2428500 - 30000) Y LMi |[01856]; mean elements Y LMi |for interval JD2432200 - 38900 are given in the Y LMi |Table; in this interval the period changed with the Y LMi |cycle of ~2100d. Blazhko effect with the period 33.4d Y LMi |[01856]; 07m <= A <= 1.9m, 0.19P <= m - M <= 0.44P. RT LMi |Min II 11.7. RU LMi |Spectrum description [09326]. RW LMi |VB A (B 15.5m B, 9", 10deg). 0.3m - 2.6m K, 7.64m - 10.71m, RW LMi |9.7m - 14.6m R, 14.1m - 18.1m B, 14.8m - 18.6m U. RW LMi |Mean brightness varies. Gaseous-dust circumstellar RW LMi |envelope. CO emission. Spectrum description [09327]. RY LMi |VB A (B 16.1m, dM2, 15", 126deg); mu = 0.14", P = 264deg. RY LMi |P0 = 215.197388s, dP0/dt = 5.6s*10**(-14)/s, A0 = 0.0440m; RY LMi |P1 = 304.4s, A1 = 0.0150m; P2 = 271.0s, A2 = 0.0134m; RY LMi |P3 = 107.6s, A3 = 0.0032m; P4 = 126.2s, A4 = 0.0028m; RY LMi |P5 = 119.8s, A5 = 0.0026m. RY LMi |Mean brightness varies by 0.05m. R Lep |P var. Max = 2398883 + 436.44d*E (JD2398000 - 2412000); R Lep |Max = 2412849 + 418.04d*E (JD2412000 - 23000); R Lep |Max = 2423300 + 441.38d*E (JD2423000 - 36000); R Lep |since JD2436000 - see Table. R Lep |A var; 5.5m <= Max <= 9.5m (Possible period is more R Lep |than 40 years [03402]). S Lep |Mean magnitude varies with the cycle of 890d. H2O maser. T Lep |SiO maser. U Lep |P var. Max = 2425084.431 + 0.58147098d*E U Lep |(JD2411000 - 25090); Max = 2425084.431 + 0.58147377d*E U Lep |(JD2425080 - 37700) [03403]; since JD2436600 - see Table. U Lep |Delta(S) = 8.5; (k - b)2 = 0.00. V Lep |Min II 9.9. Z Lep |Min II 12.0:. RR Lep |Min II 10.4. RS Lep |Min II 9.96. RU Lep |P var? RZ Lep |S 4/4. SS Lep |SB2 (Porb = 258.2d [09363]). SY Lep |VB A (B 15.2m: V, 18", 270deg). S Lib |P var. Max = 2405692 + 192.14d*E (JD2402700 - 24000); S Lib |Max = 2424141 + 194.74d*E (JD2424000 - 30500); S Lib |Max = 2431900 + 190.34d*E (JD2430500 - 37200); S Lib |Max = 2439203 + 197.61d*E (JD2437200 - 39300); S Lib |since JD2441000 - see Table. Mean value of the period is S Lib |given in the Table. A var (1.8m <= A <= 5m). W Lib |P var. Max = 2412272 + 203.76d*E (JD2412000 - 28500); W Lib |Max = 2428573 + 201.48d*E (JD2428500 - 34000); W Lib |since JD2434000 - see Table. X Lib |P var. Max = 2423500 + 165.75d*E (JD2413000 - 25000); X Lib |since JD2425000 - see Table. Y Lib |P var. Max = 2413452 + 275.7d*E (JD2413400 - 22000); Y Lib |Max = 2422273 + 272.5d*E (JD2422000 - 28000) [00458]; Y Lib |Max = 2434921 + 277.04d*E (JD2428000 - 35000); Y Lib |since JD2435000 - see Table. Z Lib |P var. Max = 2417736 + 294.5d*E (JD2407100 - 17800); Z Lib |since JD2424400 - see Table. RR Lib |P var. Max = 2409699 + 277.4d*E (JD2409600 - 15600); RR Lib |Max = 2416345 + 273.2d*E (JD2416300 - 19700); RR Lib |Max = 2421027 + 278.6d*E (JD2421000 - 27150) [00458]; RR Lib |since JD2427150 - see Table. RS Lib |P var. Max = 2413396 + 217.2d*E (JD2413300 - 20000); RS Lib |Max = 2420110 + 219.6d*E (JD2420000 - 27500) [00458]; RS Lib |Max = 2429078 + 215.6d*E (JD2427500 - 35000); RS Lib |Max = 2438196 + 219.9d*E (JD2435000 - 42600); RS Lib |since JD2441700 - see Table. RT Lib |P var. Max = 2413776 + 254.21d*E (JD2413000 - 19000); RT Lib |since JD2419000 - see Table. RU Lib |P var. Max = 2413363 + 312.0d*E (JD2413300 - 16200); RU Lib |Max = 2416807 + 322.5d*E (JD2416800 - 21000); RU Lib |Max = 2421309 + 317.0d*E (JD2421300 - 24200); RU Lib |Max = 2424804 + 311.5d*E (JD2424800 - 29800) [00458]; RU Lib |Max = 2434909 + 319.9d*E (JD2429800 - 35000); since RU Lib |JD2437700 - see Table. RV Lib |Min II 9.44. RX Lib |[A/H] = -0.5. P var. Max = 2430913.6 + 24.950d*E RX Lib |(JD2425000 - 36300) [00266]; since JD2436300 - see Table. SS Lib |Min II 10.8; d = 0.030P. ST Lib |VB A (B 14m, 14", 0deg). TV Lib |Delta(S) = 2.5. TY Lib |d = 0.019P. UW Lib |[Fe/H] = - 0.25. VV Lib |P var. Max = 2424268.474 + 0.4781418d*E VV Lib |(JD2419800 - 2425000); since JD2425000 - see Table. VW Lib |Observations given in VW Lib |[00293] contradict the elements given in the Table. VY Lib |P var? [03506].Delta(S) = 6. VZ Lib |Min II 10.55; dI = 0.000P; dII = 0.005P. P var. Min I = VZ Lib |2429022.227 + 0.358053d*E (JD2428600 - 30400) VZ Lib |[09368]; Min I = 2430899.223 + 0.358448d*E VZ Lib |(JD2430400 - 32400) [02532]; since JD2444330 - see Table. YZ Lib |Min II 12.9. AA Lib |P var? The elements are valid in the interval AA Lib |JD2427800 - 29600. AF Lib |The chart in [06286] has south on top. AP Lib |Z = 0.0486. AQ Lib |[Fe/H] = -0.60. BE Lib |The chart in [06286] is wrong. BH Lib |Recommended chart in [06286]: part III, page 50. BT Lib |Min II 12.3. BW Lib |The chart in [06286] is wrong. CG Lib |[Fe/H] = -1.82. P var. Max = 2438592.287 + 0.3068674d*E CG Lib |(JD2427800 - 39600) [07557]; since JD2439600 - see Table. CQ Lib |The coordinates in [01870] are wrong. CZ Lib |The chart in [06286], part I, page 40 is wrong. Recomended CZ Lib |chart in [06286]: part III, page 52. EH Lib |Delta(S) = 0. 9.35m <= Max < = 9.49m V; EH Lib |Max (A) = 2442162.556 + 0.273778d*E [09336]. ES Lib |Min II 7.33. EU Lib |70d <= P <= 90d. FI Lib |90d <= P <= 110d. FS Lib |OH emission. FX Lib |Spectrum description [06167,09371]. del Lib |VB A (B 11.3m, 9", 351deg; C 12.80m, 67", 90deg); Min II del Lib |4.98. P var? S Lup |VB A (B = X Lup, 13", 176deg). P var. Max = 2411950 + S Lup |347.81d*E (JD2411950 - 14000); Max = 2414040 + S Lup |339.31d*E (JD2414000 - 19000); Max = 2419135 + S Lup |345.12d*E (JD2419000 - 26000); Max = 2426038 + S Lup |336.60d*E (JD2426000 - 29500); Max = 2429743 + S Lup |345.15d*E (JD2429500 - 35000); since JD2437600 - see Table. X Lup |VB B (A = S Lup). Y Lup |P var. Max = 2424691 + 408.15d*E (JD2423000 - Y Lup |25500); Max = 2425503 + 394.81d*E (JD2425500 - Y Lup |30250); Max = 2430641 + 407.75d*E (JD2430250 - Y Lup |35000); since JD2437900 - see Table. RU Lup |Sometimes varies quasiperiodically: P1 = 3.5457d, P2 = RU Lup |3.8375 [02412]. H2O maser. RY Lup |Quasiperiodicity: P = 3.7609d [09366]. SX Lup |Min II 11.8. TY Lup |The chart in [06286] is wrong. UX Lup |[A/H] = -0.9. P var. P = 16.2403d (JD2411526 - UX Lup |14040); P = 16.2065d (JD2414040 - 24016); P = UX Lup |16.2492d (JD2424016 - 25638); P = 16.1794d UX Lup |(JD2425638 - 26449); P = 16.2241d (JD2426449 - 29693) UX Lup |[05387]. VV Lup |Close northern companion. VZ Lup |P var? Light curve shape var? CC Lup |The chart in [06286] is wrong. CW Lup |The charts in [06286] are wrong. CX Lup |Min II 12.8. CY Lup |High Max every 360d, especially faint Min 80d before CY Lup |these high Max. DG Lup |Min II 15.1. DQ Lup |The chart in [06286] is wrong. DY Lup |In [00087] the information on variability of DY Lup is DY Lup |accompanied by the coordinates of DZ Lup and vice versa. DY Lup |The chart for DY Lup in [06286] is labeled DZ Lup, the DY Lup |chart for DZ Lup in [06286] is wrong. DZ Lup |In [00087] the information on variability of DY Lup is DZ Lup |accompanied by the coordinates of DZ Lup and vice versa. DZ Lup |The chart for DY Lup in [06286] is labeled DZ Lup, the DZ Lup |chart for DZ Lup in [06286] is wrong. EL Lup |VB. ER Lup |P2 = 140d. EU Lup |The chart in [06286] is wrong. FK Lup |Min II 10.7:. FM Lup |The chart in [02385] is wrong. FR Lup |Deep Min II. FT Lup |Min II 9.98. dI = 0.025P?, dII >= 0.066P. P var. FT Lup |Before JD2439300 Min I = 2427987.310 + 0.470089d*E FT Lup |[03948]; since JD2445000 - see Table. All the observations FT Lup |are well represented also by the elements: FT Lup |Min I = 2445061.834 + 0.470083d*E - 0.114d*10**(-9)*E**2 FT Lup |[09360]. Light curve shape var? FV Lup |Min II 11.2. GG Lup |Min II 5.8. GN Lup |VB A (B 10.2m vis, 10", 98deg). GO Lup |Relatively short P. GW Lup |In the dark nebula Barnard 228. HK Lup |B - V: +1.23, +1.46. HL Lup |The initial identification with 2U 1543 - 47 is wrong. HL Lup |2U 1543 - 47 = IL Lup. HM Lup |B - V: +1.12. HN Lup |B - V: +1.55, +1.68. HO Lup |B - V: +0.70, +0.81. alf Lup |VB A (B 14.0m, 27.6", 232deg, 1901). alf Lup |Soft X-ray source. P2 = 3.145d is possible [08417]. gam Lup |SB, Porb = 2.8081d. del Lup |Less probable variant of elements: del Lup |Max = 2441045.160 + 0.14273*E. R Lyn |S 4/5E - S 6/6 - . S Lyn |VB A (B 14m, 12.6", 155deg). P var. Max = 2414564 + S Lyn |300.26d*E (JD2414500 - 27400); Max = 2434241 + S Lyn |294.42d*E (JD2427400 - 35100); Max = 2440225 + S Lyn |300.44d*E (JD2435100 - 40220); since S Lyn |JD2440220 - see Table. T Lyn |P var. Max = 2425012 + 419.0d*E (JD2412800 - 34700); T Lyn |since JD2434700 - see Table. U Lyn |H2O, OH emission. P var. Max = 2417168 + U Lyn |440.3d*E (JD2417100 - 26000) [00458]; Max = U Lyn |2435908 + 432.05d*E (JD2426000 - 36000); Max = U Lyn |2439898 + 447.1d*E (JD2436000 - 40000); since U Lyn |JD2440000 - see Table. V Lyn |Cycles 55d and 87d replace one another. Mean brightness V Lyn |varies. Y Lyn |SB. RR Lyn |VB A (B 10m, 50"). Min II 5.90; Min II = 2438051.3115 + RR Lyn |9.945074d*E; E = 0.081; Min II - Min I = 0.45P (JD2437700). RW Lyn |[Fe/H] = -1.37. RZ Lyn |Min II 10.8. SW Lyn |Min II 9.65; dI = 0.038P. P var. Min I = 2425643.323 + SW Lyn |0.6440661d*E (JD2425640 - 35850) [02742]; Min I = SW Lyn |2438795.8016 + 0.6440520d*E (JD2438380 - 840) SW Lyn |[09387]; Min I = 2440614.0107 + 0.6440729d*E SW Lyn |(JD2439500 - 40620) [00001]; Min I = 2442786.4493 + SW Lyn |0.6440677d*E (JD2440650 - 42790) [07292]; SW Lyn |since JD2442780 - see Table. SX Lyn |Min II 10.1. P var. Min I = 2428636.375 + 2.0225615d*E SX Lyn |(JD2427400 - 34700) [00519]; Min I = 2442561.424 + SX Lyn |2.0225172d*E (JD2442400 - 44000); since JD2444000 - see SX Lyn |Table. SZ Lyn |SB (Porb = 1146d, E = 0.26 [09388]). Delta(S) = 0. SZ Lyn |There is a periodical term in the elements: SZ Lyn |-0.00573d cos 2pi (EP0/P1 + 0.007); P0 = 0.120534920d, SZ Lyn |P1 = 1150d. Amplitude and shape of the light curve vary. TT Lyn |Delta(S) = 7. TV Lyn |[Fe/H] = -0.99. TW Lyn |Delta(S) = 10. P var. Max = 2418676.804 + 0.4817201d*E TW Lyn |(JD2418670 - 20155); Max = 2420155.685 + 0.4816929d*E TW Lyn |(JD2420155 - 27480); Max = 2427479.359 + 0.4817481d*E TW Lyn |(JD2427480 - 28630); TW Lyn |Max = 2428627.310 + 0.4818529d*E (JD2428620 - 37800) TW Lyn |[02819]. Since JD2445000 - see Table. TZ Lyn |Epoch of Min brightness is given. UU Lyn |Min II 11.82. UV Lyn |Min II 9.78. UZ Lyn |VR var (P = 0.065d [09392]). VV Lyn |VB A (B 11.76m, 38.6",354deg); SB; mu alpha = -0.0285S, VV Lyn |mu delta = -0.274". VW Lyn |P1 = 590s, P2 = 260s [09393]. CW Lyn |Type RRC: is also possible. S Lyr |P var. Max = 2416186 + 432.01d*E (JD2415700 - 20100); S Lyr |Max = 2420961 + 445.83d*E (JD2420900 - 26500); S Lyr |Max = 2426748 + 429.01d*E (JD2426500 - 30700); S Lyr |Max = 2432357 + 441.88d*E (JD2432000 - 34600); S Lyr |since JD2442500 - see Table. U Lyr |VB A (B 13.0m, 9.4", 182deg). P var. Max = 2418345 + U Lyr |459.22d*E (JD2418000 - 27000); since JD2432000 - see U Lyr |Table. V Lyr |OH maser. W Lyr |P var. Max = 2415578 + 198.39d*E (JD2413000 - 19000); W Lyr |Max = 2420322 + 194.99d*E (JD2419000 - 25500); W Lyr |Max = 2431326 + 198.97d*E (JD2427000 - 31500); W Lyr |Max = 2432494 + 195.11d*E (JD2431500 - 36500); W Lyr |since JD2437500 - see Table. Y Lyr |Delta(S) = 0.8. Z Lyr |P var. Max = 2418150 + 285.07d*E (JD2417500 - 22200); Z Lyr |Max = 2423600 + 291.37d*E (JD2422200 - 29500); Z Lyr |Max = 2430000 + 284.00d*E (JD2429500 - 36800); Z Lyr |since JD2436800 - see Table. RR Lyr |mu alpha = -0.11", mu delta = -0.19". [Fe/H] = -1.14; RR Lyr |Delta(S) = 6. Blazhko effect of variable RR Lyr |amplitude (practically to complete disappearance of RR Lyr |Blazhko effect); Pi = 40.8d. Variations of Max light RR Lyr |phase up to 0.14P; magnitude in Max var in the range RR Lyr |up to 0.6m, that in Min var in the range up to 0.1m RR Lyr |[03418].According to [07270], a cycle ~4 yr is present RR Lyr |in Blazhko effect amplitude changes; at the end of RR Lyr |the cycle the Blazhko effect phase changes abruptly RR Lyr |by 0.25Pi. Magnetic field strength varies with the RR Lyr |pulsational period [09339]. RR Lyr |P var. Max = 2414856.480 + 0.56682069d*E RR Lyr |(JD2414800 - 18800); Max = 2421854.052 + 0.56685169d*E RR Lyr |(JD2418800 - 26500) [09379]; Max = 2426571.3828 + RR Lyr |0.56684333d*E (JD2426500 - 32500) [09338]; Max = RR Lyr |2438215.9492 + 0.566830d*E (JD2438000 - 41000) RR Lyr |[05238]; Max = 2438215.9492 + 0.56683313d*E RR Lyr |(JD2441000 - 42900) [09338]; since JD2442900 - see Table. RS Lyr |P var. Max = 2415566 + 299.38d*E (JD2415000 - 24000); RS Lyr |Max = 2425176 + 308.08d*E (JD2424000 - 37200); RS Lyr |since JD2437200 - see Table. RT Lyr |P var. Max = 2437022 + 250.85d*E (JD2415000 - 39000); RT Lyr |since JD2439000 - see Table. RU Lyr |P var. Max = 2415983 + 370.70d*E (JD2415900 - 33000); RU Lyr |Max = 2433035 + 363.0d*E (JD2433000 - 41000); RU Lyr |since JD2441000 - see Table. RV Lyr |D = 0.015P. P var. Min = 2415949.7096 + 3.599007d*E RV Lyr |(JD2412185 - 16000); Min = 2415949.7096 + RV Lyr |3.599046d*E (JD2416000 - 21400) [00001]; RV Lyr |Min = 2432015.671 + 3.5989845d*E (JD2421400 - 32000); RV Lyr |Min = 2432015.671 + 3.5990235d*E (JD2432000 - RV Lyr |39300) [09085]; since JD2442000 - see Table. RW Lyr |OH, H2O maser. RX Lyr |P var. Max = 2416226 + 249.94d*E (JD2415000 - 28800); RX Lyr |since JD2428800 - see Table. RZ Lyr |P var. Max = 2416415.360 + 0.51127069d*E RZ Lyr |(JD2413000 - 19000) [00001]; Max = 2426161.4375 + RZ Lyr |0.51124948D*E (JD2426000 - 38000) [00323]; RZ Lyr |since JD2438000 - see Table. RZ Lyr |Blazhko effect, height of Max varies: 10.6m - 10.9m, RZ Lyr |Max (Delta(m)) = 2430904.3 + 116.654d*N + 0.01034d*N**2; RZ Lyr |Min (Delta(m)) - Max (Delta(m)) = 59.3d [03419]. RZ Lyr |[Fe/H] = -1.69; Delta(S) = 10.0. SS Lyr |P var. Max = 2421695 + 350.48d*E (JD2416000 - 22500); SS Lyr |Max = 2429991 + 355.22d*E (JD2429000 - 38000); since SS Lyr |JD2438000 - see Table. SZ Lyr |According to [05750], during JD2434665 - 35044 the SZ Lyr |amplitude was twice smaller than usual (due to the depth SZ Lyr |of Min), and a temporary phase shift by 0.5P occured. TT Lyr |d = 0.010P; Min II 9.44. TW Lyr |VB A (B 15.2m pg, 14".70deg, 1912). TY Lyr |P var. Max = 2419285 + 336.49d:*E (JD2419000 - 23700); TY Lyr |Max = 2423985 + 329.79d*E (JD2423700 - 31250); TY Lyr |since JD2438600 - see Table. TZ Lyr |VB A (B 12.29m, 2.54", 2.5deg). Min II 11.05. P var. TZ Lyr |Min I = 2420669.480 + 0.5288234d*E (JD2420000 - 38000); TZ Lyr |since JD2438000 - see Table. UX Lyr |B - V: +0.11, +0.47. UZ Lyr |d = 0.012P:. P var. Min = 2424268.474 + 1.891253d*E UZ Lyr |(JD2422500 - 25500) [02087]; since JD2425500 - see Table. AA Lyr |Min II 13.5. AH Lyr |d = 0.03P. Min II 12.1. AK Lyr |Min II 12.9. AL Lyr |P var. Max = 2427865.82 + 12.9837d*E (JD2414800 - 28000) AL Lyr |[00001]; Max = 2432889.03 + 12.98047d*E AL Lyr |(JD2428000 - 35500) [04427]; since JD2435500 - see Table. AQ Lyr |P var. Max = 2425301.592 + 0.3571721d*E AQ Lyr |(JD2425300 - 29000); Max = 2428944.739 + 0.3571285d*E AQ Lyr |(JD2429000 - 30200); Max = 2430158.976 + 0.3571611d*E AQ Lyr |(JD2430200 - 33900); Max = 2433909.178 + 0.3571861d*E AQ Lyr |(JD2433900 - 35700); during JD2435700 - 37800 - see Table. AQ Lyr |Blazhko effect? According to visual observations, AQ Lyr |0.4m <= Delta(m) <= 1.2m. AY Lyr |Cycles of supermaxima 188.9d - 212.8d. AY Lyr |Superhumps period: Ps = 0.07552d [06249]. BF Lyr |P var. Max = 2425296 + 130d*E (JD2425300 - 800); BF Lyr |During JD2429045 - 570 - see Table. BH Lyr |P var. Max = 2413712.358 + 0.6129028d*E BH Lyr |(JD2413712 - 27927); Max = 2434472.547 + 0.6128941d*E BH Lyr |(JD2434472 - 36102); since JD2436423 - see Table. BQ Lyr |Delta(S) = 0:. BV Lyr |d = 0.025P. CC Lyr |P var. Max = 2433182.7 + 24.028d*E (JD2426100 - 33400); CC Lyr |Max = 2437078.8 + 24.200d*E (JD2433400 - 37100) [00001]; CC Lyr |Max = 2439418.5 + 24.185d*E (JD2437100 - 39420) [05644]; CC Lyr |since JD2440400 - see Table. Light curve shape var? CC Lyr |[A/H] = -2.2. CV Lyr |Possible superposition of P2 = 135d. CX Lyr |P var. Max = 2418596.111 + 0.616689d*E CX Lyr |(JD2414880 - 20000); Max = 2427696.396 + 0.616669d*E CX Lyr |(JD2427530 - 30610); since JD2433000 - see Table. CX Lyr |Delta(S) = 7:. DD Lyr |P var. Max = 2425494.334 + 0.372610d*E (JD2418900 - 27600) DD Lyr |[00001]; since JD2427600 - see Table. DF Lyr |Min II 13.4. DI Lyr |P var. Max = 2437160.310 + 0.4174486d*E (JD2437160 - 39293); DI Lyr |Max = 2439293.468 + 0.4178451d*E (JD2439293 - 40768); DI Lyr |since JD2440768 - see Table. DN Lyr |P2 = 600d. DR Lyr |[Fe/H] = -1.41; Delta(S) =7.4. DU Lyr |Min II 13.3. EN Lyr |B - V: + 0.40. + 0.43. P var. Delta(m) var. EP Lyr |Max I D = 0.20P; Min II 10.36m - 10.58m, D = 0.50P; EP Lyr |Max II 10.01m - 10.10m, D = 0.70P. EP Lyr |Secondary oscillations: P2 = 45.1d, P3 = 7067d [09354]. EW Lyr |P var; nonlinear term: EW Lyr |+0.00210d*10**(-6)*E**2 (JD2426500 - 45500); EW Lyr |since JD2442000 the observations are represented also by EW Lyr |the elements: Min = 2445597.391 + 1.948763d*E [07037,00001]. EX Lyr |[Fe/H] = -0.63; Delta(S) = 2.5. EZ Lyr |VB A (B 12.3m, 14", 302deg, 1934). P var. Since EZ Lyr |JD2426577 - see Table. Delta(S) = 7.1. FG Lyr |VB A (B 14m, <10"). d = 0.035P. P var? FH Lyr |P var? FK Lyr |The identification with HDE 337663(G5) [00021] is wrong. FL Lyr |Min II 9.52, DII = 0.05P. FN Lyr |B - V: +0.15, +0.48. FO Lyr |Min II 13.7. GY Lyr |The elements describe the brightest maxima. Between them GY Lyr |there are 2 - 3 waves of smaller amplitude. Red. HP Lyr |Min II 11.0. HQ Lyr |P var, periodic term: +30d*sin(8deg*E). HT Lyr |Min II 13.3. HY Lyr |Min II 14.1. IK Lyr |Blazhko effect? IL Lyr |According to [00569], Max = 2429375.519 + 0.377620d*E, IL Lyr |M - m = 0.14P:. IO Lyr |Delta(S) = 3. IP Lyr |Min II 13.3. IW Lyr |Min II 13.3. IY Lyr |Min II 14.1. KM Lyr |Blazhko effect: Pi = 30d, 0.14P <= M - m <= 0.20P. KP Lyr |ADS 11423 C (A 8.5m, B 9.7m; AB - C 77", 208deg; D 13.1m, KP Lyr |C - D 14", 61deg, 1904). P2 = 1300d is possible. KR Lyr |P var. The light curve shape var. KT Lyr |Min II 14.9. KX Lyr |Delta(S) = 0. LQ Lyr |[Fe/H] = -1.39; Delta(S) = 7.2. LR Lyr |P var? [Fe/H] = -1.41; Delta(S) = 7.4. LT Lyr |Rapid variation (0.5m in an hour) were observed. LX Lyr |Delta(S) = 8:. LZ Lyr |P var. Min = 2425347.565 + 1.611143d*E (JD2425347 - 32119) LZ Lyr |[00569]; since JD2442870 - see Table. MN Lyr |Min II 14.1. MR Lyr |Alternative P = 0.66d:. MS Lyr |P < 0.5d? MT Lyr |Min II 16.2. MV Lyr |SB (Porb = 0.1336d [09373]). MV Lyr |Quasiperiodic fadings of different amplitude: MV Lyr |Min = 2425558 + 455.5d*E (JD2425500 - 30100); MV Lyr |Min = 2430113 + 325.3d*E (JD2430100 - 36900); MV Lyr |Min = 2436944 + 357.8d*E (JD2436900 - 44100) [09372]. MV Lyr |After JD2444100 the mean brightness MV Lyr |level became fainter by 5m; outbursts with an amplitude MV Lyr |up to 3m of 1 - 2 months duration are observed [09404]. MV Lyr |During the bright level of light, flickering up MV Lyr |to 0.4m in 5 Min in U bAnd is observed [00365]. Soft MV Lyr |X-ray source. MV Lyr |B - V: 0.00 +- 0.40; U - B: -0.86 + -1.30. MW Lyr |P var. Max = 2429521.386 + 0.3978817d*E (JD2427700 - 36000); MW Lyr |since JD2436000 - see Table. MW Lyr |Blazhko effect: Pi = 33.3d; the amplitude varies by 0.6m. MZ Lyr |Min II 14.0. NV Lyr |d = 0.02P:. NW Lyr |P var. Max = 2436483.323 + 1.6012330d*E (JD2414500 - NW Lyr |36400) [03506]; since JD2436400 - see Table. NW Lyr |B - V: +0.38, +0.86. NY Lyr |Min II 13.1. NZ Lyr |O - C vary harmonically with an amplitude +- 0.01d, NZ Lyr |Pi ~2500P. OQ Lyr |VB (B 12.1m vis, 5.3", 175deg, 1930). OS Lyr |40d <= P <= 60d. P2 = 400d - 500d is superimposed. PQ Lyr |d = 0.014P; Min II 14.9. PS Lyr |d = 0.02P:; Min II 11.4. PU Lyr |Close companions sf, s. PV Lyr |d = 0.03P:. PY Lyr |Min II 13.4. P var. Min I = 2434980.4372 + 0.38576671d*E PY Lyr |(JD2432700 - 36900) [04248]; since JD2442500 - see Table. QQ Lyr |Min II 14.6. QT Lyr |Min II 14.6. QU Lyr |Min II 13.1. V0335 Lyr |Large scatter in the light curve. V0336 Lyr |P var. Min = 2429965.283 + 1.9049105d*E (JD2429370 - 31590); V0336 Lyr |during JD2438930 - 40010 - see Table. V0337 Lyr |Large scatter in the light curve. V0348 Lyr |Min II 16.8. V0348 Lyr |The elements are valid during JD2444023 - 45232. V0350 Lyr |P var. The elements are valid during JD2438280 - 45232. V0355 Lyr |The elements are valid during JD2429322 - 45232. V0356 Lyr |VB A (B 17.5m, 10", 120deg, [00001]). V0361 Lyr |Min II 15.3, Max II 14.7, Max II - Min I = 0.70P. V0361 Lyr |The elements are valid during JD2433776 - 45232). V0374 Lyr |Faint companions np, sf. V0380 Lyr |Faint close companion nf. V0385 Lyr |Faint close companion sf. V0388 Lyr |No brightenings were observed during JD2438322 - 39289. V0389 Lyr |The elements are valid during JD2438322 - 40007. V0390 Lyr |The elements are valid during JD2439913 - 40007. V0401 Lyr |Min II 14.4:. The period may be spurious. V0403 Lyr |P var?, Pi = 500 P? V0404 Lyr |Min II 12.4. V0406 Lyr |Min II 13.0. V0409 Lyr |P var? The elements are valid during JD2434500 - 40000. V0409 Lyr |Blazhko effect? V0411 Lyr |Min II 14.4. Alternatively RRC (P = 0.291315d). V0412 Lyr |Min II 14.1; Min II - Min I = 0.48P. V0413 Lyr |Min II 14.8? V0415 Lyr |Cycle <= 150d. V0417 Lyr |Min II 16.2. P var? V0418 Lyr |P var. The elements are valid during JD2437100 - 40400. V0423 Lyr |Min II 15.5. P var? V0424 Lyr |Blazhko effect? V0428 Lyr |Min II 14.3. Apsidal motion? V0429 Lyr |Min II 14.8? V0431 Lyr |Min II 15.1. V0435 Lyr |Possibly ew with twice longer P. P may be spurious. V0462 Lyr |P var? The elements are valid during JD2439913 - 40007. V0467 Lyr |Min II 12.9. JD2415288 - 43287; the elements V0467 Lyr |are valid during JD2415288 - 43287; large scatter V0467 Lyr |on the light curve. According to [09412], during V0467 Lyr |JD2443424 - 44165 the light variation range is 12.4m - V0467 Lyr |12.6m pg, the elements are not valid. V0470 Lyr |U = 0.40", p = 7deg. P1 = 738.6s, P2 = 557.4s, P3 = 318.0s, V0470 Lyr |P4 = 291.9s, P5 = 259.1s. V0473 Lyr |P var, Delta(m) var. According to [09413], P = V0473 Lyr |1.490795d + 1.22d*10**(-6)*(JD - 2443600)/365.25d. V0473 Lyr |Cyclic P variations: P alpha = 1178.5d; Pt = 2655d. V0473 Lyr |Delta(m) varies with the period P alpha; P4 = 1063.5d V0473 Lyr |may be traced in the variations of Vr. V0473 Lyr |0.06m <= Delta(m) <= 0.36m. V0474 Lyr |P2 = 76d. V0477 Lyr |The central star of planetary nebula Abell 46. Strong V0477 Lyr |reflection effect. Depths of minima: Min I 1.42m B, V0477 Lyr |Min II ~0.1m B. V0531 Lyr |Minima observed only between JD 2448600 and 2448800. V0550 Lyr |SB, Porb = 1.0309d. alf Lyr |IR excess. bet Lyr |ADS 11745 A (B 8.6m, B7V, 46", 149deg; C 13.0m, 47", bet Lyr |248deg). Min II 3.85. P var. Nonlinear terms: bet Lyr |+3.883d*10**(-6)*E**2 - 0.10d*10**(-10)*E**3. bet Lyr |Light curve shape var. bet Lyr |Radio and X-ray source. IR excess. del 2 Lyr |Open cluster delta**2 Lyr member [02505]. R Men |Sometimes P = 120d; R Men |Sometimes P = 240d. T Men |In the Large Magellanic Cloud region; not a member of the T Men |Cloud. There is a sguare term in the elements: T Men |+8.1d*10**(-6)*E**2. U Men |VB A (B 10.4m, 0.6", 71deg, 1935.3). A var U Men |(0.8m <= A <= 2.9M). P var. Max = 2416927 + 426.9d*E U Men |(JD2415200 - 17400) [00207]; since JD2417400 - see Table. V Men |Epoch corresponds to the middle of V Men |the light curve ascending branch. W Men |The member of the Large Magellanic Cloud. RR Men |Min II 12.1. RS Men |In the Large Magellanic Cloud region; not RS Men |a member of the Cloud. RT Men |In the Large Magellanic Cloud region; not a member of RT Men |the Cloud. RU Men |In the Large Magellanic Cloud region; not a member of RU Men |the Cloud. RV Men |In the Large Magellanic Cloud region; not a member of RV Men |the Cloud. RW Men |In the Large Magellanic Cloud region; not a member of RW Men |the Cloud. TU Men |Porb = 0.1176d [09376]. Superhump TU Men |Period Ps = 0.12625d [04772]. TY Men |Min II 8.47; d I = 0.00P, d II = 0.07P. TY Men |Shape of the light curve varies. TZ Men |Min II 6.36. UX Men |Min II 9.47; Min II - Min I = 0.50045P. UX Men |One of the components may be a physical variable. WY Men |In the region of the NGC 1841 globular cluster; not a WY Men |member of the cluster. In the halo of the magellanic WY Men |clouds system. WZ Men |In the region of the NGC 1841 globular cluster, not a WZ Men |member of the cluster. In the halo of the Magellanic WZ Men |Clouds system. XX Men |In the region of the NGC 1841 globular cluster, not a XX Men |member of the cluster. In the halo of the Magellanic XX Men |Clouds system. XY Men |In the Large Magellanic Cloud region; not a member of the XY Men |Cloud. Min II 10.88; dI = 0.05P; dII = 0.00P. XZ Men |There are there oscillations simultaneously: P1 = 0.1083d XZ Men |(A1 = 0.0094m B), P2 = 0.0855d (A2 = 0.0082m B), XZ Men |P3 = 0.0955d (A3 = 0.0058m B); P2/P1 = 0.789. AN Men |Type RRC: is also possible. iot Men |Min II 6.05. R Mic |P var. Max = 2413373 + 138.60d*E (JD2413300 - 29600) R Mic |[00458]; Max = 2432745 + 137.43d*E (JD2429600 - 34700); R Mic |Max = 2435091 + 140.84d*E (JD2434700 - 37800); R Mic |since JD2437800 - see Table. S Mic |P var. Max = 2413499 + 214.5d*E (JD2413500 - 15900) [00458]; S Mic |Max = 2432102 + 208.23d*E (JD2422700 - 32200); S Mic |since JD2432200 - see Table. U Mic |OH, H2O emission. V Mic |OH, H20 emission. Y Mic |Mean brightness varies. Z Mic |(k - b)2 = 0.12; Delta(S) = 4. RR Mic |[A/H] = -1.4. P var. Max = 2433032.96 + 31.78175d*E RR Mic |(JD2415000 - 35300) [02747]; since JD2443600 - see Table. RY Mic |P var? Elements given in the Table represent observations RY Mic |in the interval JD2436100 - 40210. RY Mic |According to [00085] Max = 2428670 + 190d*E. RZ Mic |Min II 11.2. TV Mic |Min II 12.4. UZ Mic |Min II 12.4. VW Mic |In the interval JD2436600 - 840) VW Mic |Max = 2436807.248 + 0.35620d*E. Since JD2442600 - see VW Mic |Table. WY Mic |P = 0.511427d? [00001]. XZ Mic |In the interval JD2436670 - 840 Max = XZ Mic |2436731.480 + 0.449208d*E. Since JD2442630 - see Table. ZZ Mic |(k - b)2 = 021; Delta(S) = 0. P var? Max = 2437192.3131 + ZZ Mic |0.0671786d*E (JD2437180 - 460) [04308]; ZZ Mic |Max = 2439320.2162 + 0.0671575d*E (JD2439320 - 340) ZZ Mic |[05683]; since JD2440440 - see Table. ZZ Mic |Further period increase is possible [09380]. According ZZ Mic |to [07985] there are two simultaneous oscillations with the ZZ Mic |periods P1 and P2: P1 = 0.0654d, P2 = 0.0513d. ZZ Mic |P2/P1 = 0.784; A2(U) = 0.25 A1(U). AE Mic |In the interval JD2436670 - 840 Max = AE Mic |2436728.470 + 0.324142d*E. Since JD2442630 - see Table. AH Mic |Min II 13.6. AT Mic |VB (A 10.83m V, M 4.5Ve; B 10.9m V, M 4.5Ve; a = AT Mic |6.40", P = 675 yr, e = 0.60 [09381]. AT Mic |mu alpha = + 0.0216s, mu delta = -0.331" (mu, Vr, AT Mic |pi - common with AU Mic). AT Mic |Unusually high freguency of flares AT Mic |allows to suppose that both components are variable. AT Mic |The range of combined brightness variation of the AT Mic |system is given in the Table. AU Mic |mu alpha = +0.0212S, mu delta = -0.348" (mu, pi, AU Mic |Vr - common with AT Mic). SB? 0.20P <= M - m <= 0.55P. AU Mic |There are periodical light variations and also flares with AU Mic |A <= 0.5m U [08601]. AW Mic |mu alpha = +0.0077s, mu delta = -0.089". AW Mic |Shape of the light curve strongly varies. Multiperiodicity AW Mic |is possible. AX Mic |mu alpha = -0.2805s, mu delta = -1.152". In AX Mic |minimum brightness B - V = +1.42, U - B = +1.20. R Mon |Peculiar non-stellar object at the apex of the reflection R Mon |variable [09396] cometary nebula NGC 2261. Probably young R Mon |star surrounded by dust cloud. Light curve in [09394]. S Mon |In the open star cluster S Mon |NGC 2264. VB A (B 8.2m, 2.9", 213deg; 9.9m, 16.6", 14deg.) T Mon |SB (Porb> = 70 yr [09397]). [A/H] = 0.3. T Mon |There is a sguare term in the elements given in the T Mon |Table: +5.34d*10**(-6)*E**2. T Mon |Deviations from the parabola in the O - C, E diagram T Mon |have a wave-like trend. If this wave is attributed to T Mon |the light-time effect, Porb = 100 years. T Mon |The observations are also satisfied by the following T Mon |system of linear elements: Max = 2412874.56 + 27.0093d*E T Mon |(JD2405200 - 15250) [09398]; Max = 2426004.62 + 27.0180d*E T Mon |(JD2415250 - 27150); since JD2427150 - T Mon |Max = 2436137.090 + 27.0205d*E [02392]. U Mon |P var. Min = 2408897 + 92.26d*E (JD2408800 - 36210) [00368]; U Mon |since JD2437300 - see Table. U Mon |Mean magnitude varies with the period 2320d [00657]. U Mon |Spectrum investigation [02226]. V Mon |P var. Max = 2412172 + 334.5d*E (JD2412000 - 23500) [00458]; V Mon |Max = 2427870 + 332.5d*E (JD2423500 - 28200); V Mon |Max = 2429904 + 342.0d*E (JD2428200 - 30800); V Mon |Max = 2439570 + 331.6d*E (JD2430800 - 41225); V Mon |since JD2441225 - see Table. X Mon |P var. Max = 2415078 + 154.0d*E (JD2415000 - 18800); X Mon |Max = 2419758 + 149.6d*E (JD2419700 - 21000); X Mon |Max = 2421136 + 155.0d*E (JD2421000 - 24600); X Mon |Max = 2424673 + 169d*E (JD2424600 - 25600); X Mon |Max = 2425644 + 155.6d*E (JD2425600 - 26800); X Mon |Max = 2427028 + 150.7d*E (JD2427000 - 28000) [00458]; X Mon |Max = 2429521 + 155.8d*E (JD2428000 - 36300); X Mon |Max = 2438846 + 145.3d*E (JD2437800 - 38900); since X Mon |JD2440800 - see Table. The amplitude strongly varies; X Mon |sometimes irregular light variations are observed. Y Mon |P var. Max = 2415792 + 228.6d*E (JD2415300 - 19700); Y Mon |Max = 2419928 + 227.4d*E (JD2419700 - 24300) [00458]; Y Mon |Max = 2432647 + 233.3d*E (JD2424300 - 32900); Y Mon |since JD2432900 - see Table. RR Mon |P var. Max = 2417476 + 384.5d*E (JD2417400 - 19600) [00458]; RR Mon |since JD2419600 - see Table. RU Mon |Min II 11.06; D II var: 0.06P <= DII <= 0.12P; RU Mon |Min II - Min I var: 0.25P < = Min II - Min I <= 0.75P. RU Mon |P var. In the interval JD2429100 - 38409 Min I = RU Mon |2418357.0140; 3.5846794d(E - 406) - 0.429d cos alpha + RU Mon |0.06d*sin(2alpha) + 0.010d*cos(3alpha) + RU Mon |0.003d*sin(4alpha), MinII = 2418355.2220 + RU Mon |3.5846794d(E - 406) + 0.429d cos alpha + RU Mon |0.060D*sin(2alpha) - 0.010d cos*3alpha + RU Mon |0.003d*sin(4alpha) (JD2416900 - 29100); RU Mon |Min I = 2429641.567 + 3.5846391d*(E - 3554) - RU Mon |0.429d*cos(alpha) + 0.060d*sin(2alpha) + 0.010d*cos(3alpha) + RU Mon |0.003d*sin(4alpha), RU Mon |Min II = 2429639.775 + 3.5846391d(E - 3554) + RU Mon |0.429d*cos(alpha) + 0.060d*sin(2alpha) - RU Mon |0.010d*cos(3alpha) + 0.003d*sin(4alpha), where alpha = RU Mon |0.01245deg(E - 406) [03445]. RU Mon |The epochs E are being calculated for Min I from JD hel. RU Mon |2416901.205, and for Min II - from JD hel. 2416900.248. RU Mon |In the interval JD2438409 - 41743 RU Mon |Min I = 2438409.6045 + 3.584586d(E - 6000) - RU Mon |0.4290d*cos(alpha) + 0.0620d*sin(2alpha) + RU Mon |0.0107d*cos(3alpha) + 0.0026d*sin(4alpha) - RU Mon |0.00036d cos 5alpha, Min II = 2438407.8122 + RU Mon |3.584586d(E - 6000) + 0.4290d cos alpha + RU Mon |0.0620d*sin(2alpha) - 0.0107d*cos(3alpha) + RU Mon |0.0026d*sin(4alpha) + 0.00036d*cos(5alpha), RU Mon |where alpha = 0.012385deg(E - 406) [07987]. RU Mon |since JD2441743 - Min I = 2441743.2633 + RU Mon |3.584670d(E - 6930) - 0.4336d cos alpha + RU Mon |0.0634d*sin(2alpha) + 0.0111d*cos(3alpha) + RU Mon |0.0021d*sin(4alpha), Min II = 2441741.4710 + RU Mon |3.584689d(E - 6930) + 0.4336d cos alpha + RU Mon |0.0634d*sin(2alpha) - 0.0111d*cos(3alpha) + RU Mon |0.0021d*sin(4alpha), where alpha = 70.6deg + RU Mon |0.0114deg(E - 6094) [09546]. Linear elements for Min I RU Mon |epochs in 1973 - 1990 are given in the Table. RU Mon |Corresponding elements for Min II epochs are: RU Mon |Min II = 2441741.575 + 3.584567d*E. E = 0.38. RU Mon |Apsidal motion period is 285 years. RV Mon |Mean brightness varies with P = 1047d. RW Mon |Min II 9.45; d I = 0.027P, d II = 0.023P. P var. RW Mon |Min I = 2417943.687 + 1.9061012d*E (JD2417940 - 32900) RW Mon |[03450]; since JD2432900 - see Table. RX Mon |P var. Max = 2418980 + 343.2d*E (JD2416200 - RX Mon |19000); Max = 2423097 + 338.9d*E (JD2422000 - RX Mon |28500); since JD2428500 - see Table. RY Mon |VB A (B 12.29M, 28"). SS Mon |In the region of the open cluster NGC 2264. SU Mon |S 5/7 - S 6/7. P var: 69d (JD2416700 - 19100); 203.5d SU Mon |(JD2420100 - 22920); 69d (JD2423000 - 30100). SU Mon |In the intervals JD2423000 - 520 - const (11.5m), SU Mon |JD2424820 - 980 - const (11.8m). SV Mon |[A/H] = 0.2. P var. Max = 2419041.805 + 15.230721d*E SV Mon |(JD2412000 - 22000) [00025]; Max = 2422651.931 + SV Mon |15.23256d*E (JD2422600 - 23850) [09400]; Max = SV Mon |2424571.60 + 15.2513d*E (JD2423850 - 24600); SV Mon |Max = 2434045.326 + 15.2304d*E (JD2424600 - 34100); SV Mon |since JD2433000 - see Table. SX Mon |Mean brightness varies with P = 1100d. SZ Mon |VB A (B 11m - 12m, 10" [09401]). Min II 10.55. P var. SZ Mon |Min I = 2426357.1 + 32.760d*E (JD2422000 - 26400); SZ Mon |Min I = 2427861.2 + 32.708d*E (JD2426750 - 32000); SZ Mon |since JD2432800 - see Table. SZ Mon |Shape of the light curve varies. Heights of maxima and SZ Mon |depths of minima are constant. TU Mon |Min II 9.1. TV Mon |In the region of the open star cluster NGC 2237. TW Mon |Wachmann [03453] assigns the variable to the RRab TW Mon |type with the elements Max = 2433001.371 + 0.8743887*E, TW Mon |but notes a considerable dispersion of the points around TW Mon |the mean light curve obtained with this period. As the TW Mon |periods by Hessner (PH) and Wachmann (PW) are mutually TW Mon |related (1/PW ~1/PH + 1) it is more probable on account of TW Mon |the above mentioned circumstance that the variable belongs TW Mon |to cepheids. TX Mon |[A/H] = -0.3. UV Mon |The form of the light curve being unusual for RR Lyr type UV Mon |variables (Max II 13.5 at the phase 0.39P, Min II 13.8 UV Mon |at the phase 0.22P), the period may be doubtful, UV Mon |though it was found independently by two investigators UV Mon |[00380,03453]. UX Mon |Min II 8.52; dI = 0.044P. P var? UX Mon |Brightness in maximum varies with the amplitude up to 0.2m. VV Mon |Min II 9.55; dI = dII = 0.07P. VV Mon |There is a square term in the elements given in the Table: VV Mon |-0.12d*10**(-7)*E**2. VW Mon |P var. Max = 2425243.40 + 0.6041350d*E (JD2414700 - VW Mon |30700); since JD2430700 - see Table. VW Mon |In [00386,05448] And other previous works the spurious VW Mon |period value 1.532d is being accepted suggesting the VW Mon |curious nature of the variable. Serious observations are VW Mon |necessary to select the true value of the period. VX Mon |Depth of Min II 0.07m. VY Mon |In the region of the nebula IC 446. XX Mon |[A/H] = -0.2. XZ Mon |Min II 13.6; d = 0.02P:. AA Mon |[A/H] = -0.9. P var. Max = 2430788.266 + 3.938052d*E AA Mon |(JD2425300 - 34800) [03453]; since JD2434800 - see Table. AC Mon |In the region of the open cluster NGC 2323. AK Mon |P var. Max = 2425279 + 319.2d*E (JD2425200 - 28000); since AK Mon |JD2428000 - see Table. AN Mon |Min II 11.7:; d = 0.027P. AO Mon |Min II 10.16; DII = 0.14P; Min II - Min I = 0.4933P. P var. AO Mon |Min I = 2426735.333 + 1.884758d*E (JD2426700 - 40000); AO Mon |since JD2440000 - see Table. AQ Mon |Min II 10.9; DII = 0.05P; dI = 0.014P. AR Mon |Min II 9.03; d = 0.011P. AR Mon |There is a square term in the elements given in the Table: AR Mon |-1.22d*10**(-6)*E**2. AU Mon |Min II 8.2:. Shape of the light curve varies. AU Mon |Brightness in maximum varies periodically with the AU Mon |amplitude 0.2m: Max = 2443105 + 411d*E; M - m = 0.5P. AV Mon |Depth of Min II 0.04m. AW Mon |P var. Min = 2425649.053 + 20.797d*E (JD2425500 - AW Mon |26400) [09408]; Min = 2426439.340 + 20.81905d*E AW Mon |(JD2426400 - 35900) [00511]; since JD2435900 - see Table. AX Mon |Binary system with an envelope and gaseous streams. AX Mon |Porb = 232.60d [06103]. Spectrum investigation [09411]. AX Mon |Epoch of Min brightness preceeding the moment of AX Mon |conjunction for 0.25p is given in the Table; A = 0.4m U. AX Mon |Besides periodical variations, there are rapid light AX Mon |fluctuations up to 0.1m. BB Mon |Depth of Min II 0.04m. BC Mon |P var. Max = 2421240 + 275.8d*E (JD2421200 - BC Mon |25960); Max = 2428880 + 267.2d*E (JD2425960 - BC Mon |30000); since JD2430000 - see Table. BE Mon |Delta(S) = 0. BH Mon |d = 0.01p:. BM Mon |Min II 12.3. According to [09415], apsidal motion is BM Mon |possible. BO Mon |Min II 10.1. P var. Min I = 2428211.596 + 2.2251753d*E BO Mon |(JD2415000 - 36000) [00007]; since JD2436000 - see Table. BP Mon |P var? BP Mon |Elements given in the Table are valid in the interval BP Mon |JD2425600 - 29700. BT Mon |VB A (B 16.0m, 10", 0deg). BT Mon |After the outburst in 1939 the brightness varies in the BT Mon |range 16.0m - 18.7m with the elements: Min = BT Mon |2443491.7155 + 0.3338141d*E; D = 0.20p, 0 <= d < = 0.03p. BT Mon |Before the outburst in 1939, according to [09417], BT Mon |the following elements were valid: Min = 2429500.207 + BT Mon |0.3338010d*E. Emission nebula with the radius of 3.8" BT Mon |was discovered in 1981 around the nova [09148]. BX Mon |Usually was considered as mira type variable BX Mon |[09421]. In the Table the epoch of light maximum and BX Mon |the period are given according to [09419]. According BX Mon |to [09420] the Balmer emission lines originate in the BX Mon |nebulosity surrounding the symbiotic system and are BX Mon |excited by the hot component, and light variations BX Mon |are due to the orbital motion in the system. BZ Mon |d = 0.030P. In the region of the open cluster CR 106. CC Mon |In the region of the open cluster CR 106. CD Mon |P var. Max = 2427704 + 273.8d*E (JD2427400 - 30400); since CD Mon |JD2430400 - see Table. CE Mon |Min II 14.2. CF Mon |Min II 13.7; d = 0.02P:. CH Mon |d = 0.030P. CS Mon |VB A (B 13m, 9", 0deg). CT Mon |In the region of the open cluster NGC 2244. CU Mon |[A/H] = -0.2. CV Mon |In the centre of an anonymous open cluster. CV Mon |VB A (B 13.76m, 10", 270deg; C 13.72m, 14", 270deg). CV Mon |P var. Max = 2429805.142 + 5.378782d*E (JD2429360 - CV Mon |36000); since JD2436000 - see Table. DD Mon |Min II 11.3. DF Mon |The chart in [05285] is wrong, the star observed was DF Mon |not DF Mon. DN Mon |Min II 13.9. DR Mon |In the region of the open cluster Cr 106. DT Mon |P var. Max = 2425324 + 345d*E (JD2425300 - 28200) DT Mon |In the interval JD2429250 - 37700 there were cycles 119d, DT Mon |230d, 350d. DW Mon |In the region of the open cluster NGC 2286. EE Mon |P var. Max = 2425300.42 + 4.80776d*E (JD2425300 - EE Mon |27720); since JD2427720 - see Table. EH Mon |d = 0.023P. EK Mon |P var. Max = 2425302.59 + 3.95773d*E (JD2425200 - EK Mon |33000) [00387]; since JD2433000 - see Table. EP Mon |d = 0.026P. ES Mon |d = 0.02P. EW Mon |Min II 14.2. FH Mon |Depth of Min II 0.04m. FP Mon |In the region of the open cluster NGC 2353. FS Mon |Min II 11.2. FU Mon |S 6.5/7.5. FW Mon |d = 0.016P. Depth of Min II 0.04m. FX Mon |OH emission. FZ Mon |The elements should be checked. GH Mon |Min II 13.1. GP Mon |In the region of the open cluster NGC 2264. GQ Mon |In the region of the open cluster NGC 2264. GR Mon |In the region of the open cluster NGC 2264. GU Mon |Min II 12.5. GV Mon |Depth of Min II 0.04m. GX Mon |OH, H2O, SIO maser. HI Mon |Min II 9.9. HM Mon |Min II 13.6. P var. Min I = 2430110.1948 + 0.40765737d*E HM Mon |(JD2429600 - 35400) [05285]; since JD2435400 - see Table. HO Mon |d = 0.03P. HP Mon |d = 0.04P:. HR Mon |Depth of Min II 0.03m. HY Mon |Min II 12.4. IL Mon |d = 0.03P. IM Mon |Min II 6.47. IO Mon |In the region of the open cluster NGC 2264. IP Mon |In the region of the open cluster NGC 2264. IQ Mon |In the region of the open cluster NGC 2264. IR Mon |P var? IS Mon |Depth of Min II 0.05m. IX Mon |Min II 12.8. IZ Mon |Min II 12.0. KU Mon |In the region of the open cluster NGC 2264. KV Mon |In the region of the open cluster NGC 2264. KW Mon |In the region of the open cluster NGC 2264. KX Mon |In the region of the open cluster NGC 2264. KY Mon |In the region of the open cluster NGC 2264. KZ Mon |In the region of the open cluster NGC 2264. LL Mon |In the region of the open cluster NGC 2264. LM Mon |In the region of the open cluster NGC 2264. LN Mon |In the region of the open cluster NGC 2264. LO Mon |In the region of the open cluster NGC 2264. LP Mon |In the region of the open cluster NGC 2264. LQ Mon |In the region of the open cluster NGC 2264. LR Mon |In the region of the open cluster NGC 2264. LS Mon |In the region of the open cluster NGC 2264. LT Mon |In the region of the open cluster NGC 2264. LU Mon |In the region of the open cluster NGC 2264. LV Mon |In the region of the open cluster NGC 2264. LW Mon |In the region of the open cluster NGC 2264. LX Mon |In the region of the open cluster NGC 2264. LY Mon |In the region of the open cluster NGC 2264. LZ Mon |In the region of the open cluster NGC 2264. MM Mon |In the region of the open cluster NGC 2264. MN Mon |In the region of the open cluster NGC 2264. MO Mon |VB A (B 20m, 10", 356deg); in the region of the MO Mon |open cluster NGC 2264. MP Mon |In the region of the open cluster NGC 2264. MQ Mon |In the region of the open cluster NGC 2264. MX Mon |Min II 11.7. NN Mon |Min II 12.9. NS Mon |Min II 11.1. NT Mon |In the region of the open cluster NGC 2264. NU Mon |In the region of the open cluster NGC 2264. NV Mon |In the region of the open cluster NGC 2264. NW Mon |In the region of the open cluster NGC 2264. NX Mon |In the region of the open cluster NGC 2264. NY Mon |In the region of the open cluster NGC 2264. NZ Mon |In the region of the open cluster NGC 2264. OO Mon |In the region of the open cluster NGC 2264. OP Mon |In the region of the open cluster NGC 2264. OQ Mon |In the region of the open cluster NGC 2264. OR Mon |In the region of the open cluster NGC 2264. OS Mon |In the region of the open cluster NGC 2264. OT Mon |In the region of the open cluster NGC 2264. OU Mon |In the region of the open cluster NGC 2264. OV Mon |In the region of the open cluster NGC 2264. OW Mon |In the region of the open cluster NGC 2264. OX Mon |VB A (B 15m, 7", 35deg); in the region of the open OX Mon |cluster NGC 2264. OY Mon |In the region of the open cluster NGC 2264. OZ Mon |In the region of the open cluster NGC 2264. PP Mon |In the region of the open cluster NGC 2264. PQ Mon |In the region of the open cluster NGC 2264. PR Mon |The elements should be checked. PT Mon |In the region of the open cluster NGC 2264. PU Mon |In the region of the open cluster NGC 2264. PV Mon |In the region of the open cluster NGC 2264. PW Mon |In the region of the open cluster NGC 2264. PX Mon |In the region of the open cluster NGC 2264. PY Mon |In the region of the open cluster NGC 2264. QR Mon |290d <= P <= 400d. Depth of Min varies by QR Mon |0.9m with the period about 2000d. QT Mon |In the region of the open cluster NGC 2264. QU Mon |In the region of the open cluster NGC 2264. QV Mon |In the region of the open cluster NGC 2264. QW Mon |In the region of the open cluster NGC 2264. QX Mon |In the region of the open cluster NGC 2264. QY Mon |In the region of the open cluster NGC 2264. QZ Mon |In the region of the open cluster NGC 2264. V0334 Mon |In the region of the open cluster NGC 2264. V0335 Mon |In the region of the open cluster NGC 2264. V0336 Mon |In the region of the open cluster NGC 2264. V0337 Mon |In the region of the open cluster NGC 2264. V0338 Mon |In the region of the open cluster NGC 2264. V0339 Mon |In the region of the open cluster NGC 2264. V0340 Mon |In the region of the open cluster NGC 2264. V0341 Mon |In the region of the open cluster NGC 2264. V0342 Mon |In the region of the open cluster NGC 2264. V0343 Mon |In the region of the open cluster NGC 2264. V0344 Mon |In the region of the open cluster NGC 2264. V0345 Mon |In the region of the open cluster NGC 2264. V0346 Mon |In the region of the open cluster NGC 2264. V0347 Mon |VB A (B 20m, 12", 120deg); in the region of the open V0347 Mon |cluster NGC 2264. V0348 Mon |In the region of the open cluster NGC 2264. V0349 Mon |In the region of the open cluster NGC 2264. V0350 Mon |In the region of the open cluster NGC 2264. V0351 Mon |In the region of the open cluster NGC 2264. V0352 Mon |In the region of the open cluster NGC 2264. V0353 Mon |In the region of the open cluster NGC 2264. V0354 Mon |In the region of the open cluster NGC 2264. V0355 Mon |In the region of the open cluster NGC 2264. V0356 Mon |VB (3", 78deg); in the region of the open cluster V0356 Mon |NGC 2264. V0357 Mon |In the region of the open cluster NGC 2264. V0358 Mon |In the region of the open cluster NGC 2264. V0359 Mon |In the region of the open cluster NGC 2264. V0360 Mon |In the region of the open cluster NGC 2264. V0361 Mon |In the region of the open cluster NGC 2264. V0362 Mon |In the region of the open cluster NGC 2264. V0363 Mon |In the region of the open cluster NGC 2264. V0364 Mon |In the region of the open cluster NGC 2264. V0365 Mon |VB B (A = V591 Mon, B 7", 135deg); in the region of the V0365 Mon |open cluster NGC 2264. V0366 Mon |In the region of the open cluster NGC 2264. V0367 Mon |In the region of the open cluster NGC 2264. V0368 Mon |VB (9", 252deg); in the region of the open cluster V0368 Mon |NGC 2264. V0369 Mon |VB (11", 264deg); in the region of the open cluster V0369 Mon |NGC 2264. V0370 Mon |VB (8", 97deg); in the region of the open cluster V0370 Mon |NGC 2264. V0371 Mon |In the region of the open cluster NGC 2264. V0372 Mon |SC 7/7.5. V0373 Mon |In the region of the open cluster NGC 2264. V0379 Mon |d = 0.015P:. V0380 Mon |Min II 12.9; P = 1.98904166d? V0383 Mon |Min II 15.2. V0384 Mon |Min II 13.0. V0389 Mon |Min II 14.9. V0393 Mon |Min II 14.3. V0394 Mon |d = 0.02P; depth of Min II 0.04m. V0395 Mon |d = 0.03P. V0396 Mon |Min II 13.5. V0397 Mon |Min II 11.9. V0398 Mon |In the region of the open cluster NGC 2264. V0399 Mon |In the region of the open cluster NGC 2264. V0400 Mon |In the region of the open cluster NGC 2264. V0401 Mon |In the region of the open cluster NGC 2264. V0402 Mon |In the region of the open cluster NGC 2264. V0403 Mon |In the region of the open cluster NGC 2264. V0404 Mon |d = 0.02P:. V0405 Mon |In the region of the open cluster NGC 2264. V0406 Mon |In the region of the open cluster NGC 2264. V0407 Mon |In the region of the open cluster NGC 2264. V0408 Mon |In the region of the open cluster NGC 2264. V0409 Mon |In the region of the open cluster NGC 2264. V0410 Mon |In the region of the open cluster NGC 2264. V0411 Mon |In the region of the open cluster NGC 2264. V0412 Mon |In the region of the open cluster NGC 2264. V0413 Mon |In the region of the open cluster NGC 2264. V0414 Mon |In the region of the open cluster NGC 2264. V0415 Mon |In the region of the open cluster NGC 2264. V0416 Mon |In the region of the open cluster NGC 2264. V0417 Mon |In the region of the open cluster NGC 2264. V0418 Mon |In the region of the open cluster NGC 2264. V0419 Mon |In the region of the open cluster NGC 2264. V0420 Mon |In the region of the open cluster NGC 2264. V0421 Mon |In the region of the open cluster NGC 2264. V0422 Mon |In the region of the open cluster NGC 2264. V0423 Mon |In the region of the open cluster NGC 2264. V0424 Mon |In the region of the open cluster NGC 2264. V0425 Mon |In the region of the open cluster NGC 2264. V0426 Mon |VB A (B = NSV 3125 17.0m, 6", 117deg); in the region of V0426 Mon |the open cluster NGC 2264. V0427 Mon |In the region of the open cluster NGC 2264. V0428 Mon |In the region of the open cluster NGC 2264. V0429 Mon |In the region of the open cluster NGC 2264. V0430 Mon |In the region of the open cluster NGC 2264. V0431 Mon |In the region of the open cluster NGC 2264. V0432 Mon |In the region of the open cluster NGC 2264. V0433 Mon |In the region of the open cluster NGC 2264. V0434 Mon |In the region of the open cluster NGC 2264. V0435 Mon |In the region of the open cluster NGC 2264. V0436 Mon |In the region of the open cluster NGC 2264. V0437 Mon |In the region of the open cluster NGC 2264. V0438 Mon |In the region of the open cluster NGC 2264. V0439 Mon |In the region of the open cluster NGC 2264. V0440 Mon |In the region of the open cluster NGC 2264. V0441 Mon |In the region of the open cluster NGC 2264. V0442 Mon |Min II 11.6. V0443 Mon |In the region of the open cluster NGC 2264. V0444 Mon |In the region of the open cluster NGC 2264. V0445 Mon |Min II 11.3. V0446 Mon |[A/H] = -0.7. V0447 Mon |[A/H] = -1.4. V0448 Mon |Min II 9.8. V0449 Mon |d = 0.02P. V0450 Mon |Min II 12.6. V0451 Mon |Min II 14.7. V0452 Mon |Min II 12.7; d = 0.02P. V0453 Mon |Min II 11.8. V0454 Mon |Min II 12.2. V0455 Mon |Min II 15.3. V0456 Mon |Min II 13.7. V0457 Mon |Min II 14.3; d = 0.03P:. V0458 Mon |Min II 13.8. V0459 Mon |Min II 14.7. V0460 Mon |Min II 10.7. V0463 Mon |d = 0.03P; P = 2.2476768d? V0464 Mon |Min II 12.3. V0465 Mon |P var. Max = 2429642.44 + 2.71341d*E (JD2425600 - V0465 Mon |30800) [03551]; Max = 2431845.65 + 2.713212d*E V0465 Mon |(JD2430000 - 35200) [03453]; Max = 2435541.315 + V0465 Mon |2.713668d*E (JD2435200 - 41600); since JD2441600 - see V0465 Mon |Table. V0466 Mon |VB A (B 15m, 135deg). V0474 Mon |(k - b)2 = 0.32. Blazhko effect: V0474 Mon |Max(O - C) = 2441664.962 + 7.74639d*N; Min(O - C) = V0474 Mon |2441669.569 + 7.74639d*N; 0.03m <= A <= 0.37m; V0474 Mon |-0.02d <= O - C <= +0.03d. Freguency analysis gives V0474 Mon |three principal oscillations [08669]: P1 = 0.1361258d V0474 Mon |(A1 = 0.18m), P2 = 0.1337745d (A2 = 0.12m), V0474 Mon |P3 = 0.1385591d (A3 = 0.04m). V0478 Mon |In the region of the nebula IC 2169. V0479 Mon |In the region of the nebula IC 2169. V0481 Mon |In the region of the nebula IC 2169. V0482 Mon |In the region of the nebula IC 2169. V0483 Mon |In the region of the nebula IC 2169. V0486 Mon |VB A (B 18.4M, 6"). In the region of the nebula NGC 2245. V0487 Mon |In the region of the nebula NGC 2245. V0488 Mon |In the region of the nebula NGC 2245. V0489 Mon |In the region of the nebula NGC 2245. V0490 Mon |In the region of the nebula NGC 2247. V0493 Mon |In the region of the open cluster Tr 5. V0494 Mon |Depth of Min II 0.05m. V0496 Mon |Min II 12.8. V0497 Mon |8.9 - 11.8 IR. V0498 Mon |P = 2.4727818d? V0500 Mon |In the region of the open cluster NGC 2264. V0501 Mon |Min II 13.1; Min II - Min I = 0.445P; DII = 0.036P. V0503 Mon |9.2 - 10.9 IR. V0505 Mon |Min II 7.55. V0507 Mon |SB2 (P = 53.781d [09483]); d = 0.015P:. V0510 Mon |[A/H] = -0.1. V0513 Mon |Depth of Min II 0.04m. V0514 Mon |Min II 13.3. V0515 Mon |Min II 12.7. V0521 Mon |Min II 10.4. V0524 Mon |Min II 15.2. V0526 Mon |P var. Max = 2433304.284 + 2.675208d*E (JD2429300 - V0526 Mon |35170); since JD2439170 - see Table. V0527 Mon |Depth of Min II 0.05m. V0530 Mon |Min II 12.8. V0532 Mon |Min II 12.8. RRC? V0535 Mon |P var. Max = 2431846.445 + 0.3328791d*E V0535 Mon |(JD2429600 - 34060); since JD2434060 - see Table. V0535 Mon |[Fe/H] = -1.44. V0539 Mon |In the region of the open cluster NGC 2244. V0540 Mon |In the region of the nebula IC 446. V0541 Mon |In the region of the nebula IC 446. V0542 Mon |In the region of the nebula IC 446. V0543 Mon |In the region of the open cluster NGC 2244. V0544 Mon |In the region of the open cluster NGC 2244. V0545 Mon |In the region of the open cluster NGC 2244. V0546 Mon |In the region of the open cluster NGC 2244. V0547 Mon |In the region of the open cluster NGC 2244. V0548 Mon |In the region of the open cluster NGC 2244. V0549 Mon |In the region of the open cluster NGC 2244. V0550 Mon |VB A (B 17.3m, 6", 0deg ); in the region of the open V0550 Mon |cluster NGC 2244. V0551 Mon |In the region of the open cluster NGC 2244. V0552 Mon |In the region of the open cluster NGC 2244. V0553 Mon |In the region of the open cluster NGC 2244. V0554 Mon |In the region of the open cluster NGC 2244. V0555 Mon |In the region of the open cluster NGC 2244. V0556 Mon |In the region of the open cluster NGC 2244. V0557 Mon |In the region of the open cluster NGC 2244. V0560 Mon |Depth of Min II 0.05m. V0565 Mon |Connected with the diffuse nebula V0565 Mon |NGC 2313 having diameter of 10" and a faint cometary V0565 Mon |nebula. V0569 Mon |VB A (B 10.8m, 6.2", 281deg; C 10.5m, 38.3", 295deg). V0569 Mon |The range of combined light variation of A and B V0569 Mon |components is given. According to [08215], P = 0.18d. V0571 Mon |(k - b)2 = 0.32. V0571 Mon |Non-radial pulsation with variable periods: V0571 Mon |P1 = 0.0999081d (A1 = 0.052m), P2 = 0.0749998d V0571 Mon |(A2 = 0.015m) (JD2440914 - 41692) [07127]; P1 = 0.0894534d V0571 Mon |(A1 = 0.038m), P2 = 0.15988d (A2 = 0.025m), P3 = 0.106516d V0571 Mon |(A3 = 0.014m). P4 = 0.26998d (A4 = 0.012m), P5 = 0.15069d V0571 Mon |(A5 = 0.011m) (JD2441662 - 719) [09450]. V0577 Mon |VB (A 11.3m V, B 14.8m V; a = 0.312", P = 16.60 yr, e = V0577 Mon |0.38); mu alpha = +0.049S, mu beta = +0.73". V0577 Mon |Both components are probably variables. The range V0577 Mon |of combined light variation of the system is given V0577 Mon |in the Table [06146]. V0578 Mon |In the region of the open cluster NGC 2244. V0579 Mon |In the region of the open cluster NGC 2264. V0580 Mon |In the region of the open cluster NGC 2264. V0581 Mon |In the region of the open cluster NGC 2264. V0582 Mon |In the region of the open cluster NGC 2264. V0583 Mon |In the region of the open cluster NGC 2264. V0584 Mon |In the region of the open cluster NGC 2264. V0585 Mon |In the region of the open cluster NGC 2264. V0586 Mon |In the region of the open cluster NGC 2264. V0588 Mon |In the region of the open cluster NGC 2264. V0589 Mon |In the region of the open cluster NGC 2264. V0590 Mon |VB (10", 358deg); in the region of the open cluster V0590 Mon |NGC 2264. V0591 Mon |VB A (B = V365 Mon, 7", 135deg); in the region of the open V0591 Mon |cluster NGC 2264. V0593 Mon |In the region of the open cluster NGC 2264. V0594 Mon |In the region of the open cluster NGC 2264. V0595 Mon |In the region of the open cluster NGC 2264. V0596 Mon |In the region of the open cluster NGC 2264. V0597 Mon |In the region of the open cluster NGC 2264. V0598 Mon |In the region of the open cluster NGC 2264. V0599 Mon |In the region of the open cluster NGC 2264. V0600 Mon |In the region of the open cluster NGC 2264. V0601 Mon |In the region of the open cluster NGC 2264. V0602 Mon |In the region of the open cluster NGC 2264. V0603 Mon |In the region of the open cluster NGC 2264. V0604 Mon |In the region of the open cluster NGC 2264. V0605 Mon |In the region of the open cluster NGC 2264. V0606 Mon |In the region of the open cluster NGC 2264. V0607 Mon |In the region of the open cluster NGC 2264. V0608 Mon |In the region of the open cluster NGC 2264. V0609 Mon |In the region of the open cluster NGC 2264. V0610 Mon |In the region of the open cluster NGC 2264. V0611 Mon |In the region of the open cluster NGC 2264. V0612 Mon |In the region of the open cluster NGC 2264. V0613 Mon |S 3/2. V0616 Mon |Novalike outbursts were observed in 1917 (Max JD2421540) V0616 Mon |and in 1975 (Max JD2442646). In quiescent state probably V0616 Mon |ellipsoidal light variation is observed with P = 0.325d V0616 Mon |and A = 0.2m [09458], and also slower light variations V0616 Mon |with P = 7.39d [09459] or 7.8d [09460]. Spectrum description V0616 Mon |[09461,09462]. V0624 Mon |In the region of the open cluster Cr 106. V0628 Mon |In the region of the open cluster NGC 2264. V0629 Mon |In the region of the open cluster NGC 2264. V0630 Mon |VB A (B 21m, 3", 300deg); in the region of the open V0630 Mon |cluster NGC 2264. V0632 Mon |In the region of the open cluster NGC 2368. V0637 Mon |Basic oscillation with A1 = 0.05m and elements given in V0637 Mon |the Table is superimposed by the second one with V0637 Mon |A2 = 0.02m and the elements: Max = 2443496.1624 + V0637 Mon |0.19740d*E. Beat period Pb = 6.09d. V0638 Mon |VB (6.5m, 8.5m; 0.8", 178deg). V0640 Mon |In the region of the open cluster NGC 2244. V0640 Mon |Porb = 14.39604d [06103]. V0640 Mon |Irregular light variations. V0640 Mon |Probably transitional stage from a binary system of V0640 Mon |O stars to a system of WR type [04107]. V0641 Mon |VB A (B 10.91m, 21.4", 310deg; C 12.46m, 25.8", 285deg). V0641 Mon |In the region of the open cluster NGC 2264. V0642 Mon |In the region of the open cluster NGC 2264. Cluster V0642 Mon |non-member. Epoch of light minimum is V0642 Mon |given in the Table. V0645 Mon |Epoch of light minimum is given in the Table. V0741 Mon |Type ACV: is also possible. V0750 Mon |In the region of the nebula IC 2177. V0753 Mon |Type ACV: is also possible. S Mus |Marked on the chart for BO Mus. Max II = Max I, S Mus |D (Max II) = 0.15P. P var? SB 1 (Porb = 506.4d). T Mus |P2 = 1021d. V Mus |In the Coal Sack region. RV Mus |P = 128d: is possible. RW Mus |P = 130d: is possible. RY Mus |V1 (NGC 4833). RZ Mus |V2 (NGC 4833). Cluster non-member. SY Mus |Min II 11.2; Min I - Min II = 170d. SY Mus |Elements for Min I of quasiperiodic variations observed SY Mus |during JD2434910 - 41510 are given. Radio source. TU Mus |Min II 8.65. P var. Min I = 2424260.396 + 1.38728d*E TU Mus |(JD2423900 - 29300) [00039]; during JD2437380 - 41900 - see TU Mus |Table. The light curve shape var. TV Mus |Min II 11.3. TW Mus |Min II 12.4. TZ Mus |B - V: +1.22, +1.43. UW Mus |Min II 11.9. UY Mus |Min II 12.0. VW Mus |Min II 13.9. WY Mus |P var. Periodic term: +0.35d*sin(0.12deg*E). XZ Mus |Before JD2419200 Max = 2412590 + 113d*E. AB Mus |Min II 13.0. AS Mus |[A/H] = 0.5. AX Mus |P var. During JD2412550 - 19200 - see Table; during AX Mus |JD2423900 - 26100 P = 97.3d. AY Mus |Min II 10.8. Min II - Min I = 0.481P. AY Mus |The elements are valid during 1897 - 1943. In the time AY Mus |interval JD2441683 - 721 eclipses did not occur [08094]. BB Mus |P, possibly P should be doubled. BD Mus |Depth of Min II 0.05m. BE Mus |Min II 14.1. BF Mus |Min II 14.4. BK Mus |P very long P: 56d < d < 310d. BR Mus |Min II 11.25. B - V: +0.10m. BS Mus |Min II 11.5. BX Mus |Depth of Min II 0.04m. CD Mus |Min II 14.7. CS Mus |P > 120d. DW Mus |According to [08135], the spectral type is M5e, typical of DW Mus |Mira stars. Elements in [03934] were deduced from the DW Mus |observed brightness variations with P ~355d which DW Mus |was considered to be a spurious period; rapid variations DW Mus |were confirmed by 7h of photographic observations. DZ Mus |Possibly Pshould be doubled. EE Mus |In the coal sack. The flare was observed spectroscopically. EN Mus |d = 0.035P:. EP Mus |[A/H] = 0.2. According to [08136], EA, EP Mus |P = 4.15d, D = 0.05P, 11.63m - 12.60m V, Min II 11.7:. ET Mus |Alternatively possible type EW [08727,04001]. EV Mus |d = 0.09P:. EY Mus |In the Coal Sack region. EZ Mus |Alternative possible values of P 4.3032d, 4.3224d. FH Mus |Depth of Min II 0.03m. FO Mus |P var? GK Mus |Min II 15.0. GN Mus |Min II 14.2. GO Mus |Min II 15.2. GP Mus |B - V: +1.03, +1.61. KU Mus |Type RV: is also possible. alf Mus |VB A (B 13.0m, 29.3", 316deg). eta Mus |VB A (B 7.30m, 60"). tet Mus |VB (A 5.64m, B 7.5m, 5.3", 187deg); SB (Porb = 18.341B). tet Mus |Variable intensity of emission lines with respect to the tet Mus |continuum (double wave; elements in the Table are for the tet Mus |epochs of Min I variability in the UV range (lambda lambda tet Mus |1550 - 3300 A) with an amplitude about 2%, P = 1.5d and tet Mus |rapid changes (lamda lamda 1550 - 1800 A) with an tet Mus |amplitude about 3 - 5% on the time scale of 50s - 70s tet Mus |[08532]. Connected with a nebula, 80'*45'. R Nor |VB A (B 14.0m, 5.7", 268deg, 1929). P var. Max II = R Nor |2406371 + 486.94d*E (JD2406300 - 25000); Max II = R Nor |2426359 + 500.56d*E (JD2426000 - 30500); Max II = R Nor |2431377 + 489.0d*E (JD2430500 - 34500); since R Nor |JD2437600 - see Table. Like R Cen, has a doudle Max, R Nor |JD2437600 - see Table. Like R Cen, has a doudle Max, R Nor |divided by a comparatively shallow Min II. Max II is R Nor |usually brighter than Max I. D (Min I) = 0.43P, R Nor |D (Max I) = 0.70P, D(Min II) = 0.85P. S Nor |In the centre of the open cluster NGC 6087, cluster member. S Nor |[A/H] = -0.1. T Nor |P var.Max = 2414783 + 241.87d*E (JD2414700 - 28000); T Nor |Max = 2428084 + 244.93d*E (JD2428000 - 35000); T Nor |since JD2437000 - see Table. U Nor |P var. Max = 2415028.94 + 12.64084d*E (JD2415000 - 26000) U Nor |[00060]; since JD2434000 - see Table, [A/H] = -0.6. W Nor |P2 ~1300d. Y Nor |VB A (B 12.2m vis, 4.0", 156deg, 1903). Z Nor |Min II 9.6. RR Nor |Min II 9.9. RS Nor |B - V: +1.13, +1.48. RT Nor |Quasiperiodic variations: P1 ~59d, P2 ~175d [08140]. RV Nor |[A/H] = 0.8. RV Nor |There are irregularities in the light curve. SV Nor |Min II 12.6. SW Nor |d = 0.003P. SX Nor |d = 0.1P. SY Nor |VB A (B 12.8m, 2.1", 315deg, 1934). B - V: +1.16, +1.49. SY Nor |[A/H] = 0.5. SZ Nor |Min II 12.6. TT Nor |Twice longer P is possible. TU Nor |Min II 12.5. Associated with a small faint nebula. TV Nor |Min II 9.3. TW Nor |In the region of the poor open cluster Lynga 6. TW Nor |B - V: +1.79, +2.22. [A/H] = 0.2. TX Nor |Min II 12.5. TZ Nor |Min II 12.1. UV Nor |d ~0.07P. UX Nor |In Max light B - V = +0.30. UY Nor |d = 0.025P. UZ Nor |d = 0.02P. VV Nor |In the region of the cluster NGC 6152. VX Nor |Depth of Min II ~0.03m. VZ Nor |In the region of the cluster NGC 6152. Min II 14.3. WX Nor |The chart is erroneously labelled as that for WZ Nor. WX Nor |Min II 12.8. WZ Nor |The chart is erroneously labelled as that for WX Nor. WZ Nor |Min II 13.4. XY Nor |Min II 13.2. AA Nor |[A/H] = -0.1. AF Nor |In the region of the open cluster NGC 5999. AQ Nor |The chart in [06286] is wrong. AR Nor |The chart in [06286] is wrong. AT Nor |d = 0.026P:. BE Nor |Min II 14.2. BF Nor |The chart in [06286] is wrong. BH Nor |Min II 13.2. BP Nor |Close companion. CE Nor |d = 0.05P. Min II 11.8? CG Nor |The chart in [06286] is wrong. CI Nor |The chart in [06286] is wrong. CT Nor |The chart in [06286] is wrong. CX Nor |Min II 15.0. DE Nor |The chart in [06286] is wrong. DF Nor |The chart in [06286] is wrong. DO Nor |Min II 14.2. In the region of the open cluster NGC 6087. DP Nor |The chart in [06286] is wrong. DR Nor |In the region of the open cluster NGC 6087. EE Nor |The chart in [06286] is wrong. EM Nor |Min II 13.8. ET Nor |d = 0.032P. FG Nor |The chart in [06286] is wrong. FI Nor |The chart in [06286] is wrong. FK Nor |Min II 15.0. FQ Nor |According to [00060], P = 1.994d? FW Nor |Min II 14.5. GM Nor |d = 0.02P; Min II 11.01; Min II - Min I = 0.499P GM Nor |(JD2441683 - 721), Min II - Min I = 0.531P (JD2425381 - GM Nor |28402). B - V = 0.44m. GN Nor |Min II 13.3, DII = 0.16P, Min II - Min I = 0.405P GN Nor |(JD2425900). Apsidal motion: P = 500yr. GO Nor |Min II 13.7. GQ Nor |Min II 13.8. GR Nor |[A/H] = 0.9. GT Nor |d = 0.048P. GU Nor |In the region of the open cluster NGC 6067. GU Nor |B - V: +1.17, +1.40. [A/H] = 0.1. GV Nor |d = 0.03P:. GX Nor |Min II 15.0. HH Nor |VB B (A 9.9m vis, FO; B 12.6", 148deg). d = 0.05P. HI Nor |D is very small. HK Nor |Min II 12.9. HO Nor |Min II 13.2:. HW Nor |d = 0.024P. HZ Nor |P = 2.921584d is possible. IQ Nor |B - V: +1.55, +1.93. IS Nor |In the region of the open cluster NGC 6067. IT Nor |Min II 9.8. KL Nor |P >= 140d. KM Nor |P >= 170d. KQ Nor |Mira Ceti type is not excluded [04001]. KT Nor |P >= 180d. KX Nor |Min II 14.8. LO Nor |P >= 220d. LV Nor |Deep Min II. LX Nor |Possible P values: 0.60492d, 0.7851d, etc. NR Nor |Min II 15.9. NW Nor |P > 140d. NX Nor |Min II 14.4. OS Nor |Epoch of Min is given. EW/KW type is possible. OT Nor |Min II 13.7. OU Nor |Min II 15.1. OV Nor |P >= 200d. OW Nor |P >= 120d. OX Nor |P >= 110d. PQ Nor |Possibly a cepheid which is a fainter component of an PQ Nor |unresolved binary. Epoch of Max is given. PT Nor |In the region of the open cluster NGC 6067. QT Nor |HV 5388 = HV 8903. The coordinates in [00424] are wrong. QV Nor |3U 1538 - 52. No.12 [04124]. QV Nor |Epoch of Min corresponding to the X-ray eclipse is given. QV Nor |Depth of Min I 0.05m V, that of Min II 0.08m V. The period QV Nor |of X-ray pulses Px = 528.928s [04114]. A flare was observed QV Nor |with Delta(m) > 0.3m [09456]. QX Nor |4U 1608 - 52. QZ Nor |In the open cluster NGC 6067. V0367 Nor |May be not a supergiant. V0374 Nor |Type LBV: is also possible. mu Nor |In the region of the open cluster NGC 6169. U Oct |P var. Max = 2420685 + 302.00d*E (JD2414900 - U Oct |20700); Max = 2424320 + 300.74d*E (JD2422800 - U Oct |29800); Max = 2431901 + 309.60d*E (JD2429800 - U Oct |32250); Max = 2434018 + 300.70d*E (JD2432250 - U Oct |38800); since JD2438800 - see Table. X Oct |P var.Max = 2415170 + 208.40d*E (JD2415100 - X Oct |17100); Max = 2417425 + 201.24d*E (JD2417100 - X Oct |20700); Max = 2423780 + 207.95d*E (JD2422000 - X Oct |24000); Max = 2424370 + 200.18d*E (JD2424000 - X Oct |25600); since JD2425600 - see Table. Depths of minima are X Oct |stongly variable; 1.1m <= A <= 4.0m. RV Oct |Delta(S) = 10. TX Oct |Min II 12.7. UV Oct |Delta(S) = 9; (k - b)2 = 0.06. Blazhko effect: P = 80d; UV Oct |0.14P <= M - m <= 0.24P, 0.4m <= A <= 1.3m. UZ Oct |Min II 9.48; dI = 0.00P, dII = 0.05P. P var. Min I = UZ Oct |2440223.1560 + 1.1493709d*E (JD2438300 - 42000); UZ Oct |since JD2442000 - see Table. AM Oct |Min II 14.9. BE Oct |P < 20d:. BG Oct |P = 0.7490d? BK Oct |Min II 14.6. BP Oct |(k - b)2 = 0.25. CC Oct |Basic radial pulsation with P1 = 0.12490d (A1 = 0.042m) CC Oct |is superimposed by others with periods: P2 = 0.0795317d CC Oct |(A2 = 0.008m), P3 = 0.12336d (A3 = 0.014m); P4 = CC Oct |0.11068d (A4 = 0.008m), P5 = 0.12713d (A5 = 0.006m); CC Oct |P6 = 0.11815d (A6 = 0.006m). CD Oct |mu = 0.51", p = 279deg. One of the periods P = 686s CD Oct |(A = 0.01m). CE Oct |Light oscillation with P2 = 0.054511d (A2 = 0.0056m) is CE Oct |superimposed by an oscillation with P1 = 0.2100d or CE Oct |0.2660d (A1 = 0.0052m), which is due to pulsation or CE Oct |ellipsoidal variability in a close binary system. CP Oct |Variability type and spectral type (F2/F3Ib/II) do not agree. alf Oct |SB, Porb = 9.073d. R Oph |P var. Max = 2399214 + 302.1d*E (JD2399200 - 2427900) R Oph |[00458]; Max = 2427915 + 304.0d*E (JD2427900 - 34900); R Oph |Max = 2434906 + 301.5d*E (JD2434900 - 40600) [00001]; R Oph |since JD2440600 - see Table. U Oph |ADS 10428 A (B 12.26m, GOV, 20.4", 358deg). Min II 6.46. U Oph |P var. Periodic term: U Oph |+0.0120d*sin(0.0483deg*E + 4.7833deg). V Oph |P var. Max = 2411155 + 296.73d*E (JD2411000 - 24000); V Oph |Max = 2424198 + 302.46d*E (JD2424000 - 28000); V Oph |since JD2428000 - see Table. W Oph |P var. Before JD2420500 Max = 2415186 + W Oph |335.07d*E; Max = 2420870 + 325.33d*E (JD2420500 - W Oph |24700); since JD2424700 - see Table. X Oph |VBA (A = 0.34", Porb = 485.3 yr; B - 9m, K1III, 0.4", X Oph |142deg, 1980). X Oph |The range of the combined brightness is given. X Oph |P var. Max = 2416416 + 336.61d*E (JD2416400 - 26000); X Oph |Max = 2426161 + 331.28d*E (JD2426000 - 32500); Max = X Oph |2432788 + 335.50d*E (JD2432500 - 38000); X Oph |since JD2438000 - see Table. Y Oph |SB1? Porb = 2612d? P var. Before JD2427000 Y Oph |Max = 2408694.77 + 17.11884d*E; since Y Oph |JD2432000 - see Table. [A/H] = -0.2. Z Oph |P var. Max = 2411896 + 349.0d*E (JD2411800 - 21000) Z Oph |[00458]; Max = 2420962 + 352.1d*E (JD2421000 - 25000); Z Oph |Max = 2425183 + 347.4d*E (JD2425000 - 31000); Z Oph |Mean elements after JD2431000 - see Table. RR Oph |P var. Nonlinear term: -0.009282d*E2. RS Oph |Previous outbursts: 1898, 1933, 1958. RS Oph |According to [07575], in 1972 - 1973 there were semiregular RS Oph |variations (Delta(m) ~0.5M, P = 50D - 70D). RT Oph |P var. Before JD2426500 Max = 2417452 + RT Oph |429.00d*E; Max = 2426461 + 422.67d*E (JD2426500 - RT Oph |34000); since JD2434500 - see Table. OH, H2O maser. RU Oph |P var. Before JD2422000 Max = 2417388 + RU Oph |200.95d*E; Max = 2422011 + 203.62d*E (JD2422000 - RU Oph |27300); Max = 2427298 + 200.5d*E (JD2427300 - 29000); RU Oph |Max = 2429305 + 203.88d*E (JD2429000 - 33000); RU Oph |during JD2433000 - 40500 - see Table. RV Oph |d = 0.015P; Min II 9.56, DII = 0.09P. The light curve RV Oph |share var. RW Oph |P var. Max = 242494 + 247.86d*E (JD2425000 - 34000). RW Oph |The Table gives mean elements. RX Oph |OH, H2O maser. RY Oph |P var. Max = 2415235 + 151.05d*E (JD2414700 - 24000); RY Oph |Max = 2424152 + 149.69d*E (JD2424000 - 31000); Max = RY Oph |2431339 + 150.94d*E (JD2431000 - 40000); RY Oph |since JD2440000 - see Table. RZ Oph |d = 0.030P. SS Oph |P var. Before JD2432500 Max = 2417330 + 179.88d*E. ST Oph |(k - b)2 = 0.03. SV Oph |The elements are valid since JD2422000. SW Oph |VB A (B 12.0m vis, 2.4", 91deg, 1943). d = 0.02P. P var. SW Oph |Min = 2418880.528 + 2.445948d*E (JD2418880 - 26200) SW Oph |[00001]; Min = 2431235.216 + 2.446086d*E (JD2427900 - SW Oph |33500) [02389]; since JD2434000 - see Table. SX Oph |d = 0.03P. SZ Oph |P var. Before JD2428400 Min = 2421057.556 + 3.708454d*E; SZ Oph |since JD2442000 - see Table. TT Oph |[Fe/H] = -0.5. TW Oph |P2 = 2000d:. Associated with a nebula of variable TW Oph |brightness [03479]. UU Oph |d = 0.024P. P var? UX Oph |P var. Max = 2426041 + 117.34d (JD2406430 - 28040); UX Oph |since JD2433100 - see Table. VW Oph |P var. Mean elements are given. During JD2422500 - 30600 VW Oph |Max = 2430554 + 282.69d*E. WW Oph |Epoch of Min is given. The chart in [06286] is wrong. WZ Oph |Min II 9.82. XX Oph |A symbiotic object featuring deep fadings XX Oph |of long duration [09489]. AH Oph |H2O maser. AQ Oph |The chart in [06286] is wrong. BE Oph |The data in [00278] refer to another star. BF Oph |SB? P var? since JD2430000 - see Table. BN Oph |80d <= P <= 250d. DM Oph |P var. P = 220d (1893 - 1910), P = 216d (1914 - 1928). DQ Oph |P = 35d is possible. FK Oph |V2 (NGC 6273). GM Oph |V12 (NGC 6284). GR Oph |P var. Max = 2415425 + 136d*E (1893 - 1908); GR Oph |during 1910 - 1928 - see Table. IL Oph |P2 = 140d:. IW Oph |In the field of the globular cluster NGC 6293, IW Oph |possible cluster member. KM Oph |In the field of the globular cluster NGC 6304, field star. KO Oph |In a dark nebula. KQ Oph |P2 = 1500d. KR Oph |P2 > 5000d. OU Oph |V70 (NGC 6266). PU Oph |VB (A = V29 (NGC 6266), the data are in the Table; B = V28 PU Oph |(NGC 6266), 16.6m - 17m, 4B, 4.8", 7deg), B: RRAB, PU Oph |Max = 2433423.52 + 0.49749d*E, M - m = 0.15P. V0378 Oph |Min II 14.2. In the region of the open cluster CR 359. V0378 Oph |Epoch of Max is given. V0380 Oph |Porb = 0.16d. Blue. V0391 Oph |In the region of the open cluster CR 359. P var? V0391 Oph |Before JD2427000 Min = 2425501.425 + 2.89558d*E [00432]; V0391 Oph |since JD2441500 - see Table. V0392 Oph |Red. V0402 Oph |P var. Max = 2425364 + 154d*E (JD2425350 - 670); V0402 Oph |since JD2425670 - see Table. V0413 Oph |Delta(S) = 3. Blazhko effect? V0414 Oph |B - V: +0.41, +0.77. V0423 Oph |In the region of the open cluster CR 359. V0426 Oph |Outbursts separated by 17d - 55d [08079]; in 1976 - 77 the V0426 Oph |cycle was 32.3d. Outside outbursts 12.7m - 13.3m, waves V0426 Oph |with a cycle of 20 - 30 Min and slower variations. V0438 Oph |H20 Maser. V0439 Oph |B - V: +0.63, +0.97. V0442 Oph |Porb = 0.14056d. V0445 Oph |VB A (B 13.04m y, 21"nf). (k - b)2 = 0.35; Delta(S) = 2. V0445 Oph |According to [05692], Blazhko effect (Pi > 2000d). V0449 Oph |P var. Before JD243900 Min = 2428696.465 + V0449 Oph |1.243078d*E; Min = 2442959.607 + 1.243095d*E V0449 Oph |(JD2439000 - 43000); since JD2443000 - see Table. V0451 Oph |Min II 8.31; Min II - Min I = 0.494P; DII = 0.12P. V0452 Oph |Delta(S) = 5:. V0455 Oph |P var? The Table gives mean elements which need V0455 Oph |confirmation. V0456 Oph |Min II 10.5. P var. Before JD2436100 Min = V0456 Oph |2428422.341 + 1.015986d*E [00476]; since JD2441800 - see V0456 Oph |Table. V0465 Oph |B - V: +0.68, +1.10. P var? V0471 Oph |Very red. V0478 Oph |B - V: +0.86, +1.33. [A/H] = -0.7. V0478 Oph |The elements need confirmation. V0487 Oph |D <= 0.14P. In the region of the open cluster Cr 359. V0496 Oph |In the region of the open cluster Cr 359. V0501 Oph |Min II 11.1. V0502 Oph |Min II 8.81. P var. Since JD2434500 - see Table. V0506 Oph |Min II 12.0. In the region of the open cluster Cr 359. V0508 Oph |Min II 10.59. V0509 Oph |In the region of the open cluster Cr 359. V0511 Oph |Min II 13.7. In the region of the open cluster Cr 359. V0515 Oph |Max = 2425600 + 300d*E (JD2425600 - 26700); P = 140d V0515 Oph |(JD2426700 - 27300); during JD2427300 - 30200 - see Table. V0516 Oph |In the region of the globular cluster NGC 6304. V0517 Oph |In the region of the globular cluster NGC 6304. V0521 Oph |P = 164d (JD2415000 - 24600); P2 - 4000d. V0526 Oph |Min II 13.6. V0527 Oph |Min II 14.8. V0532 Oph |P >= 6000d. V0533 Oph |P >= 80d. V0534 Oph |d = 0.03P. V0535 Oph |d = 0.025P. V0536 Oph |d = 0.04P:. V0537 Oph |Min II 12.8. V0540 Oph |d = 0.05P; Min II 13.4. V0541 Oph |[A/H] = -1.0. In the region of the globular cluster V0541 Oph |NGC 6401; cluster non-member? V0543 Oph |Min II 13.6. V0549 Oph |Min II 14.0. V0550 Oph |Min II 13.0. V0554 Oph |[A/H] = -1.1. V0555 Oph |Sharp and flat maxima. Blazhko effect? V0557 Oph |Min II 15.7. In the region of the open cluster Cr 359. V0558 Oph |B - V: +0.57, +0.68. [Fe/H] = -1.48. According to [09037], V0558 Oph |P = 0.299d. V0564 Oph |[Fe/H] = -1.37. Epoch of Min is given. P var. Nonlinear V0564 Oph |term: +0.0073d*(E + 10)**2. V0565 Oph |P = 0.3957d is possible. Photoelectric observations of V0565 Oph |1968 contradict the elements [05746]. V0566 Oph |dI = 0.048P; Min II 7.89, dII = 0.06P. P var. Before V0566 Oph |JD2440500 Min = 2436744.4200 + 0.40964091d*E [08287]; since V0566 Oph |JD2440500 - see Table. V0567 Oph |(k - b)2 = 0.22; Delta(S) = 0. According to [07984], V0567 Oph |Max = 2441134.467 + 0.1300729d*E. V0568 Oph |Red. V0570 Oph |VB A (B 16.3m, 5", 90deg). V0572 Oph |In the region of the open cluster Cr 359. V0573 Oph |d = 0.034P. In the region of the open cluster Cr 359. V0574 Oph |P2 ~500d. V0577 Oph |Min II 11.9. Min II - Min I = 0.583P. DII = 0.050P. V0577 Oph |e = 0.22. V0580 Oph |VB A (B 15.5m, 0.2'). V0585 Oph |A long-period variation is superimposed? V0586 Oph |In the region of the open cluster Cr 359. V0590 Oph |Min II 13.6. V0592 Oph |Max = 2427227 + 78d*E (JD2426100 - 29400); V0592 Oph |during JD2429400 - 30150 - see Table. V0592 Oph |After intervals of irregular variability the periodicity V0592 Oph |resumes without phase shift. V0605 Oph |Epoch of Min is given. V0618 Oph |Min II 14.7:. V0636 Oph |d = 0.030P. V0683 Oph |P var. The light curve shape varies. V0687 Oph |P may be twice longer. V0693 Oph |Blazhko effect? [05692]. V0695 Oph |P var? The light curve shape varies. V0698 Oph |P var? since JD2442950 - see Table. V0700 Oph |B - V: +0.49, +0.50. [Fe/H] = -2.10. V0716 Oph |Delta(S) = 7. V0720 Oph |VI (NGC 6171). Cluster non-member. V0722 Oph |P var. Max = 2437089.456 + 0.6190385d (JD2419900 - 37100) V0722 Oph |[07806]; since JD2436700 - see Table. V0729 Oph |P var. Max = 2437492.766 + 0.4685794d*E (JD2423500 - 37800) V0729 Oph |[03560]; since JD2437400 - see Table. V0732 Oph |Unusual light curve (sharp Max; primary Min; broad Max; V0732 Oph |secondary Min 15.2). V0734 Oph |P var. Max = 2420636.497 + 0.562489d*E (JD2420600 - V0734 Oph |29100); during JD2429100 - 37150 - see Table. V0735 Oph |Min II 10.6. V0737 Oph |P = 374d is possible. V0767 Oph |According to [00104], waves with Delta(m) = 0.3m - 1.4m vis V0767 Oph |of 50d - 110d duration; mean brightness var, V0767 Oph |Delta(m) ~0.4m in 800d - 1000d. V0782 Oph |Very red. V0784 Oph |B - V: +0.26, +0.56. The period should be checked. V0786 Oph |Red. V0788 Oph |Blazhko effect? Pi = 115d. V0799 Oph |P = 215d is possible. V0802 Oph |Red. V0816 Oph |B - V: +0.25, +0.63. V0822 Oph |Blazhko effect? V0823 Oph |In the region of the open cluster IC 4665. V0825 Oph |In the region of the open cluster IC 4665. V0829 Oph |Blazhko effect? Pi = 165d. V0832 Oph |Red. V0838 Oph |P2 ~500d is possible. V0839 Oph |mu = 0.041", ro = 292deg. Min II 9.38. V0840 Oph |VB A (B 12m, 16", 116deg). V0841 Oph |Max = 2396146. V0843 Oph |SN Kepler. Max 2307193. Gaseous remnant. V0844 Oph |Min II 14.9. V0845 Oph |VB A (B 15.7m). V0847 Oph |Min II 13.1. V0848 Oph |Min II 13.4. V0851 Oph |Max = 2425828 + 95d*E (JD2425600 - 29700); V0851 Oph |during JD2429700 - 34250 - see Table. V0854 Oph |According to [08116], the spectrum V0854 Oph |resembles that of a T Tau - type star. V0868 Oph |Min II 13.6. In the region of the open cluster Cr 359. V0870 Oph |In the region of the open cluster Cr 359. V0872 Oph |P = 0.825d is possible. V0878 Oph |Min II 16.5. In the region of the open cluster Cr 359. V0911 Oph |P2 = 81d, P3 = 114d. P4 > P3? Standstills up to 100d. V0919 Oph |VB A (B sp). V0920 Oph |Min II 15.9. V0924 Oph |Min II 16.4. V0929 Oph |d = 0.050P. V0934 Oph |E type is possible. V0936 Oph |In the region of the open cluster Cr 359. V0938 Oph |Min II 15.3. In the region of the open cluster Cr 359. V0940 Oph |Min II 15.6. V0941 Oph |Min II 16.5. V0943 Oph |Min II 16.4. In the region of the open cluster Cr 359. V0945 Oph |Min II 15.1. In the region of the open cluster Cr 359. V0947 Oph |Min II 14.5. In the region of the open cluster Cr 359. V0952 Oph |P = 0.954d is possible. V0954 Oph |In the region of the open cluster Cr 359. Min II 14.9. V0954 Oph |According to [03500], const, V = 12.86m, B - V = +1.36m, V0959 Oph |P var? Max = 2429785.419 + 0.084857d*E V0959 Oph |(JD2429785 - 845) [02757]; during JD2443719 - 732 - see V0959 Oph |Table; other possible elemente: V0959 Oph |Max = 2443726.469 + 0.07786d*E. V0960 Oph |In the region of the open cluster Cr 359. V0963 Oph |Min II 15.1. In the region of the open cluster Cr 359. V0968 Oph |[Fe/H] = -1.48. In the region of the open cluster Cr 359. V0969 Oph |Min II 13.8:. In the region of the open cluster Cr 359. V0977 Oph |In the region of the globular cluster NGC 6426. V0978 Oph |In the region of the globular cluster NGC 6426. V0979 Oph |V11 (NGC 6426). Cluster non-member. V0980 Oph |In the the region of globular cluster NGC 6426. V0980 Oph |P = 0.25740d is possible. V0983 Oph |In the region of the open cluster Cr 359. V0986 Oph |In July 1980 Vr varied with P = 0.179d, 0.147d, 0.225d, V0986 Oph |and possibly 0.097d, but there were no spectrum variations, V0986 Oph |and the photometric P = 0.323d was not noticeable in Vr. V0986 Oph |SB? Porb = 15d - 20d; there is also excess power V0986 Oph |at low frequences in the photometric data. Earlier V0986 Oph |studies revealed photometric periods 0.284d - 0.4d V0986 Oph |and violation of periodicity. V0987 Oph |d = 0.02P. Min II 14.6. In the region of the open cluster V0987 Oph |Cr 359. V0998 Oph |In the region of the globular cluster NGC 6171. V0999 Oph |In the region of the globular cluster NGC 6171. V1000 Oph |Blazhko effect? V1002 Oph |Min II 15.2. V1002 Oph |RRC type with twice shorter P is possible. V1004 Oph |Blazhko effect? V1010 Oph |Min II 6.46. P var. P = 0.661464d (JD2415000 - 25000) V1010 Oph |[05738]; since JD2425000 - see Table, nonlinear term: V1010 Oph |-3.87d*10**(-10)*E**2. Min I var.The light curve shape and V1010 Oph |the depth of Min I var. V1011 Oph |Blazhko effect? V1015 Oph |D <= 0.23P, d < 0.02P; Min II 14.5. V1017 Oph |[Fe/H] = -1.25. P var? Max = 2437433.935 + 0.2343d*E V1017 Oph |(JD2437433 - 514) [03625]. During V1017 Oph |JD2442954 - 45140 - see Table. V1017 Oph |According to [09037], P = 0.361d. V1018 Oph |Possibly eclipsing. V1021 Oph |Delta(m) var. B - V: +0.42, +0.62. V1022 Oph |d = 0.06P:; Min II 15.95. V1024 Oph |Max = 2437433.559 + 0.5914d*E (JD2437433 - 514) V1024 Oph |[03625]. During JD2442954 - 45140 - see Table. V1024 Oph |RR(B) type is possible; P = 0.371d satisfies the V1024 Oph |observations during JD2442954 - 44407. V1026 Oph |Max = 2437433.562 + 0.6563d*E (JD2437433 - 514) V1026 Oph |[03625]. During JD2442954 - 45140 - see Table. V1028 Oph |Blazhko effect? V1032 Oph |P > 1.0d is not excluded. V1033 Oph |Max = 2437433.714 + 0.4845d*E (JD2437433 - 514) V1033 Oph |[03625]. During JD2442954 - 45140 - see Table. V1035 Oph |Max = 2437433.388 + 0.6100d*E (JD2437433 - 514) V1035 Oph |[03625]; during JD2442954 - 45140 - see Table. V1039 Oph |P = 0.3166d is possible. V1040 Oph |The light curve shape var. V1041 Oph |[Fe/H] = -1.06. V1042 Oph |The light curve shape var. Max = 2437433.633 + 0.5528d V1042 Oph |(JD2437433 - 514) [03625]. During JD2442954 - 45140 - see V1042 Oph |Table. V1052 Oph |Max = 2437433.537 + 0.7546d*E (JD2437433 - 514) V1052 Oph |[03625]; during JD2442954 - 45140 - see Table. V1054 Oph |VB Wolf 630AB (A 9.76m V, 12.47mu; B 9.78m V; A = 0.22", V1054 Oph |Porb = 1.71665 yr; C = Wolf 629, 11.70m V,14.75mu, V1054 Oph |dM4, 72", D = vB8, 16.7m V, 221", common mu). mu = 1.19", V1054 Oph |ro = 222deg. Lx/Lopt(V) = 0.05. V1072 Oph |P var. Max = 2439025.31 + 0.444715d*E (JD2438500 - 39025); V1072 Oph |since JD2442800 - see Table. V1075 Oph |Red. V1077 Oph |P var. Max = 2438614.40 + 0.373926d*E (JD2438200 - 700); V1077 Oph |Max = 2442871.516 + 0.37384d*E (JD2442810 - 910): V1077 Oph |Max = 2442983.345 + 0.373911d*E (JD2442920 - 3330); V1077 Oph |since JD2443330 - see Table. V1089 Oph |VB AB (B 16.4m, 2", 45deg). V1099 Oph |Red. V1100 Oph |Red. V1111 Oph |OH, H2O, SiO maser. V1120 Oph |Min II 14.3. V1121 Oph |Soft X-ray source. V1135 Oph |[Ca/H] = -0.74. V1141 Oph |P var? The light curve shape var? V1142 Oph |P var? The light curve shape var? V1146 Oph |P = 185.2d is possible. V1153 Oph |P = 153.0d is possible. V1157 Oph |B - V: +0.42, +0.66. V1161 Oph |P = 0.49d is possible [06438]. V1168 Oph |P var? The light curve shape var? V1170 Oph |P = 360d: is possible [06438]. V1174 Oph |P var? The light curve shape var? V1176 Oph |P = 269.0d is possible. V1179 Oph |P var? The light curve shape var? V1185 Oph |Other possible elements: Max = 2435630 + 177d*E [00001]. V1195 Oph |One more Max 2435637 (1956). Type M is possible. V1203 Oph |P = 315d is possible [06438]. V1204 Oph |P = 144d: or P = 191d: are possible. V1235 Oph |UV type is possible. V1240 Oph |P = 0.42136d is possible. V1244 Oph |The light curve shape var? V1258 Oph |P var? V1261 Oph |The light curve is not typical for the P in the Table [06438]. V1262 Oph |The light curve is not typical for the P in the Table [06438]. V1276 Oph |[Ca/H] = -0.1. V1296 Oph |[Ca/H] = -0.9. V1299 Oph |The light curve shape var? V1300 Oph |P = 235d: is possible. V1305 Oph |Min II 17.9:. V1307 Oph |The light curve shape var? Spurious period? [06438]. V1323 Oph |P var? V1332 Oph |[Ca/H] = -0.64. V1348 Oph |The light curve shape var? V1355 Oph |The light curve shape var? V1403 Oph |P = 215d? V1423 Oph |The light curve shape var? V1426 Oph |P var? V1451 Oph |P = 179.4d? V1474 Oph |P = 127d:? V1491 Oph |P = 328.0d? V1492 Oph |The light curve shape var? V1505 Oph |P = 86d:? V1512 Oph |The light curve shape var? V1526 Oph |P = 0.29745d? V1532 Oph |P = 144.4d? V1534 Oph |P = 198.8d? V1548 Oph |The minor planet (336) Lacadiera. V1554 Oph |P = 136.0d? V1568 Oph |P = 275.5d? V1571 Oph |P var? V1573 Oph |Type E? V1583 Oph |P - spurious? V1616 Oph |Type E? V1628 Oph |The light curve shape var? V1637 Oph |[Ca/H] = -0.44. V1661 Oph |The light curve shape var? V1666 Oph |P = 154.2d? V1676 Oph |Close optical companion? V1682 Oph |P = 118.0d? V1687 Oph |Type CW? V1702 Oph |P = 121d? V1705 Oph |P var? V1710 Oph |P = 0.37422d? V1731 Oph |The light curve shape var? V1736 Oph |P = 143.8d?, P = 244.5d? V1744 Oph |P = 191.6d? V1748 Oph |A var. Type CW? V1754 Oph |P = 128.4d? V1768 Oph |The light curve shape var? V1775 Oph |Type EW? V1793 Oph |P = 170d:? V1803 Oph |The star is not SVS 438. V1805 Oph |The light curve shape var? V1811 Oph |Min II 17.9:. V1814 Oph |P = 160.4d? V1822 Oph |P var? V1829 Oph |P = 143.2d? V1840 Oph |V 12 (NGC 6333 = M9). Cluster member. V1841 Oph |The light curve shape var? V1845 Oph |V7 (NGC 6333 = M9). Cluster member. V1853 Oph |The light curve shape var? V1860 Oph |[Ca/H] = -0.49. V1861 Oph |P = 142.0d? V1864 Oph |V3 (NGC 6333 = M9). Cluster member. V1886 Oph |The light curve shape var? V1889 Oph |P = 316.0d? V1895 Oph |The light curve shape var? V1905 Oph |P = 149.0d? V1919 Oph |P = 102.8d?, P = 227.0d? V1939 Oph |P = 330.0d? V1946 Oph |The light curve shape var? V1952 Oph |P = 248.0d? V1953 Oph |P = 199d:?, P = 235d:? V1954 Oph |P = 159.6d? V1973 Oph |P = 0.24154d? V1989 Oph |A var? V1990 Oph |P = 121d:? V1991 Oph |The light curve shape var? V1994 Oph |P = 170.0d? V1998 Oph |P = 270.5d? V2002 Oph |The light curve shape var? V2003 Oph |[Ca/H] = -0.96. V2009 Oph |V5 (NGC 6356). Cluster member. V2010 Oph |[CA/H] = -0.79. V2016 Oph |[CA/H] = -0.96. V2042 Oph |P var. Max = 2430146.478 + 0.5385d*E (JD2429100 - V2042 Oph |30202); since JD2436700 - see Table. V2045 Oph |The chart in [05159] is wrong. V2048 Oph |SB2 [06598]. In the region of the open cluster Cr 359. V2048 Oph |Along with irregular light variations typical for be stars V2048 Oph |there are rapid flares with the amplitudes up to 1.8m V2048 Oph |(lambda eff = 5800 A) [06150]. It is not excluded that the V2048 Oph |flares occur on a fainter companion of the system. V2051 Oph |Usually - 15.0m with strong flickering of brightness V2051 Oph |(up to 0.4m is 5 minutes) and rare flares. At the same V2051 Oph |time the eclipses are observed with depth to 2.5m with the V2051 Oph |elements: Min = 2444787.32124 + 0.062427865d*E [09550]; V2051 Oph |D = 0.0088P:, d = 0.0065P. V2058 Oph |In the dark nebula in the rho Oph region. V2059 Oph |In the dark nebula in the rho Oph region. V2061 Oph |In the region of the globular cluster NGC 6171 (M 107). V2062 Oph |In the dark nebula in the rho Oph region. V2063 Oph |The minor planet (64) Angelina. V2064 Oph |In the dark nebula in the rho Oph region. V2101 Oph |In a dark nebula. V2102 Oph |In the region of the globular cluster NGC 6293. V2105 Oph |Vr = 100 km/s. V2106 Oph |<Vr> = -102 km/s. V2108 Oph |H2O, SiO maser. V2112 Oph |The primary oscillation with A1 = 0.0172m V2112 Oph |(see Table) is superimposed by the secondary one V2112 Oph |(A2 = 0.0061m) with the elements: V2112 Oph |Max = 2444114.531: + 0.1449461d*E. V2116 Oph |X-ray pulsar. The pulse period is decreasing: 135s (1971), V2116 Oph |112.076s (1979), 109.668s (1980) [09553]. The spin-period V2116 Oph |may be twice longer. V2118 Oph |Probably rapidly rotating single spotted F type star. V2118 Oph |Max brightness epoch is given. V2119 Oph |In the region of the globular cluster V2119 Oph |NGC 6284. Not a member of the cluster. V2120 Oph |V6 (NGC 6284). In the region of the globular cluster V2120 Oph |NGC 6284. Not a member of the cluster. V2121 Oph |V10 (NGC 6284). In the region of the globular cluster V2121 Oph |NGC 6284. Not a member of the cluster. V2122 Oph |In the region of the globular cluster NGC 6284. Not V2122 Oph |a member of the cluster. V2123 Oph |V11 (NGC 6284). In the region of the globular cluster V2123 Oph |NGC 6284. Not a member of the cluster. V2124 Oph |In the region of the globular cluster NGC 6284. Not V2124 Oph |a member of the cluster. V2391 Oph |Porb = 88.13yr. Component B is a suspected variable star V2391 Oph |(NSV 24260) and may be the cause of variations. V2561 Oph |Not a supernova. tet Oph |SB1 (Porb = 11.44d [06597]). tet Oph |The basic oscillation (see Table) is superimposed by tet Oph |oscillations with the periods: P1 = 0.092551d, tet Oph |P2 = 0.069452d, P3 = 0.0555d, P4 = 0.0464d, P02 = tet Oph |0.137255d, P13 = 0.13845d, P24 = 0.13990d, P03 = 0.09185d. khi Oph |SB 1 (Porb = 138.8d [09558]). ome Oph |P = 1.5d? R Ori |SC 5/9.5 E. P var. Max = 2399420 + 378d*E R Ori |(JD2395600 - 99500); Max = 2412687 + 378.1d*E R Ori |(JD2403200 - 12700); Max = 2414230 + 366.5d*E R Ori |(JD2413800 - 16800); Max = 2417943 + 378.1d*E R Ori |(JD2416800 - 21350); Max = 2421352 + 384.9d*E R Ori |(JD2421350 - 24100); since JD2424100 - see Table. S Ori |VB A (B 10.9m, 47", 228deg). SiO maser. P var. S Ori |Max = 2404538 + 412.00d*E (JD2404520 - 13600); S Ori |Max = 2414014 + 427.15d*E (JD2414000 - 19150); S Ori |Max = 2419567 + 416.11d*E (JD2419570 - 22890); S Ori |Max = 2423312 + 407.10d*E (JD2423320 - 31050); S Ori |Max = 2431454 + 438.53d*E (JD2431500 - 39000) S Ori |[03765]; since JD2439000 - see Table. T Ori |In the T-association of the Orion nebula. Connected with T Ori |a cometary nebula. U Ori |SiO, OH, H2O maser. P var. Max = 2409881 + 374.5d*E U Ori |(JD2409800 - 15900); Max = 2415871 + 367.9d*E U Ori |(JD2415900 - 21000); Max = 2421016 + 376.0d*E U Ori |(JD2421000 - 29300); Max = 2428164 + 368.3d*E U Ori |(JD2428100 - 32900) [00960]; U Ori |Max = 2433336 + 372.7d*E (JD2432900 - 43800); U Ori |since JD2443800 - see Table. V Ori |P var. Max = 2413656 + 264.8d*E (JD2411800 - 18700); V Ori |Max = 2418987 + 271.7d*E (JD2418700 - 24600); V Ori |Max = 2424695 + 263.7d*E (JD2424600 - 29400) V Ori |[00960]; Max = 2430769 + 269.9d*E (JD2430700 - 36200); V Ori |since JD2437700 - see Table. W Ori |Mean magnitude varies with P = 2450d. Z Ori |Min II 9.9; d = 0.013P. RS Ori |P var. Max = 2428073.205 + 7.566836d*E (JD2416500 - RS Ori |33000); since JD2435000 - see Table. RT Ori |Mean magnitude varies with P = 3200d. RU Ori |In the region of the nebula IC 434. RV Ori |In the region of the nebula IC 434. RW Ori |In the region of the nebula IC 434. RX Ori |In the region of the Orion nebula T-association. RZ Ori |In the region of the Orion nebula T-association. SS Ori |In the region of the Orion nebula T-association. ST Ori |In the region of the Orion nebula T-association. SU Ori |In the region of the Orion nebula T-association. SV Ori |In the region of the Orion nebula T-association. SW Ori |In the region of the Orion nebula T-association. SX Ori |In the region of the Orion nebula T-association. SY Ori |In the region of the Orion nebula T-association. SZ Ori |In the region of the Orion nebula T-association. TT Ori |In the region of the Orion nebula T-association. TU Ori |In the region of the Orion nebula T-association. TV Ori |In the region of the Orion nebula T-association. TW Ori |In the region of the Orion nebula T-association. TX Ori |VB A (B = TY Ori, 42.4", 45deg); in the region of TX Ori |the nebula IC 434. TY Ori |VB B (A = TX Ori); in the region of the nebula IC 434. TZ Ori |In the region of the nebula IC 434. UW Ori |Min II 11.6. UY Ori |In the region of the Orion nebula T-association. UZ Ori |In the region of the Orion nebula T-association. VV Ori |Min II 5.50; dI = 0.055P; dII = 0.064P. VV Ori |There is third component in the system VV Ori |(Porb = 119.09d [08045]). VW Ori |In the region of the Orion nebula T-association. VX Ori |In the region of the Orion nebula T-association. VY Ori |VB A (B = 16.6mV, 16", 135deg). In the region of the Orion VY Ori |nebula T-association. VZ Ori |In the region of the Orion nebula T-association. WW Ori |In the region of the Orion nebula T-association. WX Ori |VB A (B 17m, 11", 10deg). In the region of the Orion nebula WX Ori |T-association. WY Ori |In the region of the Orion nebula T-association. WZ Ori |In the region of the Orion nebula T-association. XX Ori |In the region of the Orion nebula T-association. XY Ori |In the region of the Orion nebula T-association. XZ Ori |The periodicity in light variations is possible. XZ Ori |In the region of the Orion nebula T-association. YY Ori |Emission. In the region of the Orion nebula T-association. YZ Ori |In the region of the Orion nebula T-association. ZZ Ori |In the region of the Orion nebula T-association. AA Ori |In the region of the Orion nebula T-association. AB Ori |In the region of the Orion nebula T-association. AC Ori |In the region of the Orion nebula T-association. AE Ori |In the region of the Orion nebula T-association. AF Ori |In the region of the Orion nebula T-association. AG Ori |VB A (B 16.4mV, 16", 185deg). In the region of the Orion AG Ori |nebula T-association. AH Ori |In the region of the Orion nebula T-association. AI Ori |In the region of the Orion nebula T-association. AK Ori |In the region of the Orion nebula T-association. AL Ori |In the region of the Orion nebula T-association. AM Ori |VB A (B 20.3mV, 3.5", 320deg). In the region of the Orion AM Ori |nebula T-association. AN Ori |In the region of the Orion nebula T-association. AO Ori |In the region of the Orion nebula T-association. AP Ori |In the region of the Orion nebula T-association. AQ Ori |In the region of the Orion nebula T-association. AR Ori |VB A (B 2", 240deg). In the region of the Orion nebula AR Ori |T-association. AS Ori |In the region of the Orion nebula T-association. AT Ori |In the region of the Orion nebula T-association. AU Ori |In the region of the Orion nebula T-association. AV Ori |VB A (B 18.7mV, 6", 305deg). In the region of the nebula AV Ori |T-association. AW Ori |In the region of the Orion nebula T-association. AX Ori |In the region of the Orion nebula T-association. AY Ori |In the region of the Orion nebula T-association. AZ Ori |In the region of the Orion nebula T-association. BB Ori |In the region of the Orion nebula T-association. BC Ori |In the region of the Orion nebula T-association. BD Ori |In the region of the Orion nebula T-association. BE Ori |In the region of the Orion nebula T-association. BF Ori |In the region of the Orion nebula T-association. BG Ori |In the region of the nebula IC 434. BH Ori |In the region of the Orion nebula T-association. BK Ori |P var. Max = 2422016 + 338.0d*E (JD2413550 - 22100); BK Ori |Max = 2428880 + 326.5d*E (JD2422300 - 28880); BK Ori |Max = 2429940 + 345.3d*E (JD2428880 - 29940); BK Ori |Max = 2432892 + 327.7d*E (JD2429940 - 32900); BK Ori |Max = 2438800 + 346.3d*E (JD2432900 - 38800); BK Ori |since JD2438800 - see Table. BM Ori |In the region of the Orion nebula T-association. In the BM Ori |cluster NGC 1976. Orion Trapezium BM Ori |member: teta**1 Ori B (A = V1016 Ori; B 8.7", 32deg; BM Ori |C 5.13m, 13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.05P; BM Ori |Min II 7.98. Shape of the light curve and depths of minima BM Ori |vary. BO Ori |In the region of the Orion nebula T-association. BP Ori |In the region of the Orion nebula T-association. BS Ori |In the region of the Orion nebula T-association. BT Ori |In the region of the Orion nebula T-association. BU Ori |In the region of the Orion nebula T-association. BV Ori |In the region of the Orion nebula T-association. BW Ori |In the region of the Orion nebula T-association. BX Ori |In the region of the Orion nebula T-association. BY Ori |In the region of the Orion nebula T-association. BZ Ori |In the region of the Orion nebula T-association. CC Ori |In the region of the Orion nebula T-association. CD Ori |In the region of the Orion nebula T-association. CE Ori |In the region of the Orion nebula T-association. CF Ori |In the region of the Orion nebula T-association. CG Ori |In the region of the Orion nebula T-association. CH Ori |In the region of the Orion nebula T-association. CI Ori |VB A (B 9.70m, 12.9", 88deg). CM Ori |P var? CN Ori |Porb = 0.163097d. CN Ori |Light curve is superposed by oscillations with CN Ori |the following elements: Max0 = 2444941.5032 + CN Ori |0.163097d*E (A0 = 0.2m), Max1 = 2444941.573 + CN Ori |0.15946d*E (A1 = 0.1m) [09471]. CN Ori |Sometimes smaller rapid light oscillations are also CN Ori |observed with periods 24.3s - 29.5s (A<1%). CO Ori |Member of the T-association CO Ori |CO Ori. VB A (B 13m, 1", 280deg). CP Ori |Min II 11.2. P var [02545]. CT Ori |SRD? P = 68d? [09496]. CW Ori |Min II 13.2. DK Ori |In the region of the Orion nebula T-association. DK Ori |VB (ro < 3"). DL Ori |In the region of the Orion nebula T-association. DM Ori |In the region of the Orion nebula T-association. DN Ori |Min II 9.9; d = 0.026P. P var. Min I = 2428497.51 + DN Ori |12.9649d*E (JD2425200 - 28600); since DN Ori |JD2435570 - see Table. DY Ori |B - V: +0.58, +1.72. EG Ori |d = 0.086P. P var? EQ Ori |Min II 10.3. P var. Min I = 2425889.706 + 1.74608d*E EQ Ori |(JD2425600 - 26700) [02839]; Min I = 2429219.467 + EQ Ori |1.74611d*E (JD2427700 - 31000) [00001]; EQ Ori |since JD2431000 - see Table. ER Ori |VB A (B 13.6", 0deg). Min II 9.97. P var. Min I = ER Ori |2426336.6485 + 0.4233955d*E (JD2426330 - 33920) ER Ori |[00279]; Min I = 2434765.6306 + 0.42340620d*E ER Ori |(JD2433920 - 35475) [02278]; Min I = 2436508.7851 + ER Ori |0.4234009d*E (JD2435475 - 40000) [03787]; ER Ori |since JD2440000 - see Table. Shape of the light curve ER Ori |varies. ET Ori |Min II 11.3. P var? EW Ori |Min II 10.5; Min II - Min I = 0.529P. EW Ori |In the region of the open cluster CR 70. EW Ori |In [00007] Min II are accepted to be Min I, and vice EW Ori |versa (Min II - Min I = 0.47P). EW Ori |For decisive choice of the Min I epoch photoelectric EW Ori |observations are necessary. P var? Min II = EW Ori |2429974.810 + 6.9368005d*E [00007]; since EW Ori |JD2430000 - see Table. EY Ori |Min II 9.54; d = 0.003P. In the region of the Orion EY Ori |nebula T-association. P var. EY Ori |Min I = 2427310.420 + 16.787450d*E [00007]; EY Ori |since JD2427500 - see Table. EZ Ori |In the region of the Orion nebula T-association. FF Ori |Min II 10.3. FH Ori |d = 0.035P. P var. FI Ori |VB A (B 10.5m, 5", 323deg). FI Ori |Shape of the light curve varies, probably periodically FI Ori |[03790,05475]. FK Ori |P var. Min = 2427773.390 + 1.947447d*E (JD2426900 - FK Ori |37500); since JD2437500 - see Table. FL Ori |P var. Min = 2427452.271 + 1.550971d*E (JD2427450 - FL Ori |29600) [03115]; Min = 2430400.649 + 1.55093d*E FL Ori |(JD2429600 - 30400);Min = 2432517.755 + 1.550991d*E FL Ori |(JD2430400 - 32900); Min = 2434459.571 + 1.550965d*E FL Ori |(JD2432900 - 35050); Min = 2436649.568 + 1.550995d*E FL Ori |(JD2435050 - 40600); since JD2440600 - see Table. FO Ori |Min II 9.7; d = 0.005P. FR Ori |Min II 11.1. FT Ori |Min II 9.60; DII = 0.08P; Min II - Min I = 0.73P. P var. FT Ori |Min I = 2433009.553 + 3.150404d*E (JD2426380 - 38000) FT Ori |[02758]; since JD2438000 - see Table. FT Ori |The period of apsidal motion 520 +- 100 years [07358]. FU Ori |Member of FU Ori T-association. In the dark globule B35. FU Ori |Connected with a bright cometary nebula and the bright FU Ori |hydrogen nebula S 280. Light maximum was in summer FU Ori |1937. IN 1980 - 10.6m B. FZ Ori |Min II 11.2. GG Ori |Min II 11.1; Min II - Min I = 0.427P. GP Ori |SC 7/8- . GQ Ori |VB A (B 9.7m, 31", 324deg). GW Ori |In the T-association CO Ori. GX Ori |In the T-association CO - Ori. GY Ori |In the T-association CO - Ori. GZ Ori |In the region of the Orion nebula T-association. HH Ori |In the region of the Orion nebula T-association. HI Ori |In the T-association CO - Ori. HK Ori |In the T-association CO - Ori. HK Ori |Connected with a bright cometary nebula. CO, CH, OH HK Ori |emission. HL Ori |In the region of the Orion nebula T-association. HM Ori |In the T-association CO - Ori. HN Ori |In the region of the Orion nebula T-association. HO Ori |In the region of the Orion nebula T-association. HP Ori |In the region of the Orion nebula T-association. HQ Ori |In the region of the Orion nebula T-association. HR Ori |In the region of the Orion nebula T-association. HS Ori |In the region of the Orion nebula T-association. HT Ori |In the region of the Orion nebula T-association. HU Ori |In the region of the Orion nebula T-association. HV Ori |In the region of the Orion nebula T-association. HW Ori |In the region of the Orion nebula T-association. HX Ori |In the region of the Orion nebula T-association. HY Ori |In the region of the Orion nebula T-association. HZ Ori |In the region of the Orion nebula T-association. II Ori |In the region of the Orion nebula T-association. IK Ori |In the region of the Orion nebula T-association. IL Ori |In the region of the Orion nebula T-association. IM Ori |In the region of the Orion nebula T-association. IN Ori |In the region of the Orion nebula T-association. IO Ori |In the region of the Orion nebula T-association. IP Ori |In the region of the Orion nebula T-association. IQ Ori |In the region of the Orion nebula T-association. IR Ori |In the region of the Orion nebula T-association. IS Ori |In the region of the Orion nebula T-association. IT Ori |In the region of the Orion nebula T-association. IU Ori |In the region of the Orion nebula T-association. IV Ori |In the region of the Orion nebula T-association. IW Ori |In the region of the Orion nebula T-association. IX Ori |In the region of the Orion nebula T-association. IY Ori |In the region of the Orion nebula T-association. IZ Ori |In the region of the Orion nebula T-association. KK Ori |In the region of the Orion nebula T-association. KL Ori |In the region of the Orion nebula T-association. KM Ori |In the region of the Orion nebula T-association. KN Ori |In the region of the Orion nebula T-association. KO Ori |In the region of the Orion nebula T-association. KP Ori |In the region of the Orion nebula T-association. KQ Ori |In the region of the Orion nebula T-association. KR Ori |In the region of the Orion nebula T-association. KS Ori |In the region of the Orion nebula T-association. KT Ori |In the region of the Orion nebula T-association. KU Ori |In the region of the Orion nebula T-association. KV Ori |In the region of the Orion nebula T-association. KW Ori |In the region of the Orion nebula T-association. KX Ori |In the region of the Orion nebula T-association. KY Ori |In the region of the Orion nebula T-association. KZ Ori |In the region of the Orion nebula T-association. LL Ori |In the region of the Orion nebula T-association. LM Ori |In the region of the Orion nebula T-association. LN Ori |In the region of the Orion nebula T-association. LO Ori |In the region of the Orion nebula T-association. LP Ori |In the region of the Orion nebula T-association. LQ Ori |In the region of the Orion nebula T-association. LR Ori |In the region of the Orion nebula T-association. LS Ori |In the region of the Orion nebula T-association. LT Ori |In the region of the Orion nebula T-association. LU Ori |In the region of the Orion nebula T-association. LV Ori |In the region of the Orion nebula T-association. LW Ori |In the region of the Orion nebula T-association. LX Ori |In the region of the Orion nebula T-association. LY Ori |In the region of the Orion nebula T-association. LZ Ori |VB B (A 10.3m; B 14.1", 219deg). In the region of the LZ Ori |Orion nebula T-association. MM Ori |In the region of the Orion nebula T-association. MN Ori |In the region of the Orion nebula T-association. MO Ori |In the region of the Orion nebula T-association. MP Ori |In the region of the Orion nebula T-association. MQ Ori |In the region of the Orion nebula T-association. MR Ori |In the region of the Orion nebula T-association. MS Ori |In the region of the Orion nebula T-association. MT Ori |In the region of the Orion nebula T-association. MU Ori |In the region of the Orion nebula T-association. MV Ori |In the region of the Orion nebula T-association. MW Ori |In the region of the Orion nebula T-association. MX Ori |In the region of the Orion nebula T-association. MY Ori |In the region of the Orion nebula T-association. MZ Ori |In the region of the Orion nebula T-association. NN Ori |In the region of the Orion nebula T-association. NO Ori |In the region of the Orion nebula T-association. NP Ori |In the region of the Orion nebula T-association. NQ Ori |In the region of the Orion nebula T-association. NR Ori |In the region of the Orion nebula T-association. NS Ori |In the region of the Orion nebula T-association. NT Ori |In the region of the Orion nebula T-association. NU Ori |In the region of the Orion nebula T-association. In the NU Ori |nebula NGC 1982. Dust shell. NV Ori |In the region of the Orion nebula T-association. NW Ori |In the region of the Orion nebula T-association. NX Ori |In the region of the Orion nebula T-association. NY Ori |VB B (A = V566 Ori; B 5", 135deg). In the region of the NY Ori |Orion nebula T-association. NZ Ori |In the region of the Orion nebula T-association. OO Ori |In the region of the Orion nebula T-association. OP Ori |In the region of the Orion nebula T-association. OQ Ori |In the region of the Orion nebula T-association. OR Ori |In the region of the Orion nebula T-association. OT Ori |In the region of the Orion nebula T-association. OU Ori |In the region of the Orion nebula T-association. OV Ori |In the region of the Orion nebula T-association. OW Ori |In the region of the Orion nebula T-association. OX Ori |In the region of the Orion nebula T-association. OY Ori |In the region of the Orion nebula T-association. OZ Ori |In the region of the Orion nebula T-association. PP Ori |In the region of the Orion nebula T-association. PQ Ori |In the region of the nebula IC 434. PR Ori |In the region of the Orion nebula T-association. PS Ori |In the region of the Orion nebula T-association. PT Ori |In the region of the Orion nebula T-association. PU Ori |In the region of the nebula IC 434. PV Ori |In the region of the Orion nebula T-association. PW Ori |In the region of the Orion nebula T-association. PX Ori |<Vr> = + 298 km/s [09511]. In the region of the Orion PX Ori |nebula T-association. PY Ori |In the region of the Orion nebula T-association. PZ Ori |In the region of the Orion nebula T-association. QQ Ori |In the region of the Orion nebula T-association. QR Ori |In the region of T-association FU Ori. QT Ori |P var? Elements given in the Table are valid in the QT Ori |interval JD2429640 - 35550. V0340 Ori |Epoch of Min brightness is given. V0343 Ori |Min II 11.0. Shape of the light curve and depth of V0343 Ori |Min II vary. V0347 Ori |In the region of the Orion nebula T-association. V0348 Ori |In the region of the Orion nebula T-association. V0349 Ori |In the region of the Orion nebula T-association. V0353 Ori |In the region of the Orion nebula T-association. V0354 Ori |In the region of the Orion nebula T-association. V0355 Ori |In the region of the Orion nebula T-association. V0356 Ori |In the region of the Orion nebula T-association. V0357 Ori |In the region of the Orion nebula T-association. V0358 Ori |In the region of the Orion nebula T-association. V0359 Ori |In the region of the Orion nebula T-association. V0359 Ori |Epoch of Min HEI line intensity is given. V0359 Ori |According to [09512], P = 14.612d. V0360 Ori |In the region of the Orion nebula T-association. V0361 Ori |VB C (A 4.8m; B 6.1m, 52.4", 93deg; C 129", 97deg). V0361 Ori |In the region of the Orion nebula T-association. V0362 Ori |In the region of the Orion nebula T-association. V0363 Ori |In the region of the Orion nebula T-association. V0364 Ori |In the region of the Orion nebula T-association. V0365 Ori |In the region of the Orion nebula T-association. V0366 Ori |In the region of the Orion nebula T-association. V0367 Ori |In the region of the Orion nebula T-association. V0368 Ori |In the region of the Orion nebula T-association. V0369 Ori |In the region of the Orion nebula T-association. V0370 Ori |In the T-association CO - Ori. V0371 Ori |mu = 0.28", ro = 238deg. V0372 Ori |In the region of the Orion nebula T-association. V0373 Ori |In the region of the Orion nebula T-association. V0374 Ori |In the region of the Orion nebula T-association. V0375 Ori |In the region of the Orion nebula T-association. V0376 Ori |In the region of the Orion nebula T-association. V0377 Ori |In the region of the Orion nebula T-association. V0378 Ori |In the region of the Orion nebula T-association. V0379 Ori |In the region of the Orion nebula T-association. V0380 Ori |In the nebula NGC 1999. In the region of the Orion V0380 Ori |nebula T-association. Spectrum description V0380 Ori |[04002]. OH, CH emission. V0381 Ori |In the region of the Orion nebula T-association. V0382 Ori |P var. MAX = 2431146 + 227.8d*E (JD2429300 - 31200); V0382 Ori |Mean period is given in the Table (JD2428100 - 33700). V0383 Ori |In the region of the Orion nebula T-association. V0384 Ori |In the region of the Orion nebula T-association. V0385 Ori |In the region of the Orion nebula T-association. V0386 Ori |In the region of the Orion nebula T-association. V0387 Ori |In the region of the Orion nebula T-association. V0388 Ori |In the region of the Orion nebula T-association. V0389 Ori |In the region of the Orion nebula T-association. V0390 Ori |In the region of the Orion nebula T-association. V0391 Ori |In the region of the Orion nebula T-association. V0393 Ori |In the region of the Orion nebula T-association. V0394 Ori |In the region of the Orion nebula T-association. V0395 Ori |In the region of the Orion nebula T-association. V0396 Ori |In the region of the Orion nebula T-association. V0397 Ori |In the region of the Orion nebula T-association. V0398 Ori |In the region of the Orion nebula T-association. V0399 Ori |In the region of the Orion nebula T-association. V0400 Ori |In the region of the Orion nebula T-association. V0401 Ori |In the region of the Orion nebula T-association. V0402 Ori |In the region of the Orion nebula T-association. V0403 Ori |In the region of the Orion nebula T-association. V0404 Ori |In the region of the Orion nebula T-association. V0405 Ori |In the region of the Orion nebula T-association. V0406 Ori |In the region of the Orion nebula T-association. V0407 Ori |In the region of the Orion nebula T-association. V0408 Ori |In the region of the Orion nebula T-association. V0409 Ori |In the region of the Orion nebula T-association. V0410 Ori |In the region of the Orion nebula T-association. V0411 Ori |In the region of the Orion nebula T-association. V0412 Ori |In the region of the Orion nebula T-association. V0413 Ori |In the region of the Orion nebula T-association. V0414 Ori |In the region of the Orion nebula T-association. V0415 Ori |In the region of the Orion nebula T-association. V0416 Ori |In the region of the Orion nebula T-association. V0417 Ori |In the region of the Orion nebula T-association. V0418 Ori |In the region of the Orion nebula T-association. V0419 Ori |In the region of the Orion nebula T-association. V0420 Ori |In the region of the Orion nebula T-association. V0421 Ori |In the region of the Orion nebula T-association. V0422 Ori |In the region of the Orion nebula T-association. V0423 Ori |In the region of the Orion nebula T-association. V0424 Ori |In the region of the Orion nebula T-association. V0425 Ori |In the region of the Orion nebula T-association. V0426 Ori |In the region of the Orion nebula T-association. V0427 Ori |In the region of the Orion nebula T-association. V0428 Ori |In the region of the Orion nebula T-association. V0432 Ori |Delta(S) = 0. V0435 Ori |P var. Max = 2430350 + 186d*E (JD2429600 - 30730); V0435 Ori |Max = 2431373 + 186d*E (JD2431370 - 3250) [02279]; V0435 Ori |since JD2434000 - see Table. V0436 Ori |In the T-association CO Ori. V0437 Ori |In the T-association CO Ori. V0438 Ori |In the T-association CO Ori. V0439 Ori |In the T-association CO Ori. V0441 Ori |In the T-association CO Ori. V0442 Ori |VB A (B 16.6m, 20", 73deg). In the T-association CO Ori. V0443 Ori |In the T-association CO Ori. V0444 Ori |In the T-association CO Ori. V0445 Ori |In the T-association CO Ori. V0446 Ori |In the T-association CO Ori. V0447 Ori |In the T-association CO Ori. V0448 Ori |In the T-association CO Ori. V0449 Ori |In the T-association CO Ori. V0449 Ori |In [08289] was considered as an EW type variable with the V0449 Ori |elements: Min I = 2430259.622 + 0.441990d*E V0449 Ori |(JD2430250 - 5550), 14.8m - 15.7m pg. V0450 Ori |In the T-association CO Ori. V0452 Ori |In the T-association CO Ori. V0453 Ori |In the T-association CO Ori. V0454 Ori |In the T-association CO Ori. V0455 Ori |In the T-association CO Ori. V0456 Ori |In the T-association CO Ori. V0457 Ori |In the T-association CO Ori. V0458 Ori |In the T-association CO Ori. V0460 Ori |In the T-association CO Ori. V0461 Ori |In the T-association CO Ori. V0463 Ori |In the T-association CO Ori. V0464 Ori |In the T-association CO Ori. V0465 Ori |In the T-association CO Ori. V0466 Ori |In the region of the Orion nebula T-association. V0467 Ori |In the T-association CO Ori. V0468 Ori |In the region of the Orion nebula T-association. V0470 Ori |In the region of the Orion nebula T-association. Star V0470 Ori |Pi 1411. Near to WY Ori = Pi 1396. V0473 Ori |In the region of the Orion nebula T-association. V0474 Ori |In the region of the Orion nebula T-association. V0475 Ori |In the region of the Orion nebula T-association. V0476 Ori |In the region of the open cluster lambda Ori. V0477 Ori |In the region of the open cluster lambda Ori. V0478 Ori |In the region of the Orion nebula T-association. V0479 Ori |In the region of the Orion nebula T-association. In the V0479 Ori |infrared A>1.5m. V0480 Ori |In the region of the Orion nebula T-association. In the V0480 Ori |infrared A>1.5m. V0481 Ori |In the region of the Orion nebula T-association. V0482 Ori |In the region of the Orion nebula T-association. V0484 Ori |In the region of the Orion nebula T-association. V0484 Ori |In the infrared A>1.0m. V0485 Ori |In the region of the Orion nebula T-association. V0485 Ori |In the infrared A>1.0m. V0486 Ori |In the region of the Orion nebula T-association. V0487 Ori |In the region of the Orion nebula T-association. V0489 Ori |In the region of the Orion nebula T-association. V0489 Ori |In the infrared A>1.0m. V0490 Ori |In the region of the Orion nebula T-association. V0490 Ori |In the infrared A>1.0m. V0491 Ori |In the region of the Orion nebula T-association. V0491 Ori |In the infrared A>1.0m. V0492 Ori |In the region of the Orion nebula T-association. V0492 Ori |Northern component of the close pair of infrared stars. V0492 Ori |In the infrared A = 1m. V0493 Ori |In the region of the Orion nebula T-association. V0493 Ori |In the infrared A>1.0m. V0494 Ori |In the region of the Orion nebula T-association. V0495 Ori |In the region of the Orion nebula T-association. V0495 Ori |Close binary (ro = 0.24"). It is unknown which of the V0495 Ori |components varies. V0496 Ori |In the region of the Orion nebula T-association. V0496 Ori |In the infrared A>1.0m. V0497 Ori |In the region of the Orion nebula T-association. V0497 Ori |In the infrared A>1.0m. V0498 Ori |In the region of the Orion nebula T-association. V0500 Ori |In the region of the Orion nebula T-association. V0501 Ori |In the region of the Orion nebula T-association. V0502 Ori |In the region of the Orion nebula T-association. V0504 Ori |Min II 15.4. V0505 Ori |In the region of the nebula IC 434. V0507 Ori |In the region of the nebula IC 434. V0508 Ori |In the region of the nebula IC 434. V0509 Ori |In the region of the nebula IC 434. V0510 Ori |In the region of the nebula IC 434. V0511 Ori |In the region of the nebula IC 434. V0514 Ori |In the region of the nebula IC 434. V0516 Ori |Max = 2430325 + 139d*E (JD2430250 - 5350); P = 70d V0516 Ori |(JD2435350 - 550). V0519 Ori |Min II 12.9. V0522 Ori |In the region of the nebula IC 434. V0523 Ori |In the region of the nebula IC 434. V0525 Ori |Min II 14.7. V0526 Ori |In the region of T-association FU Ori. V0529 Ori |Nova Ori 1678? V0529 Ori |Recurrent outburst was possibly observed at 1894 [02866]. V0529 Ori |Earlier the object was considered as nova Ori [1667 V0529 Ori |2862, 2863, 2867, 2868], its existence being considered V0529 Ori |as doubtful [03813]. V0537 Ori |In the region of the open cluster lambda Ori. V0538 Ori |In the region of the Orion nebula T-association. V0539 Ori |In the region of the Orion nebula T-association. V0540 Ori |In the region of the Orion nebula T-association. V0541 Ori |In the region of the Orion nebula T-association. V0542 Ori |In the region of the Orion nebula T-association. V0544 Ori |In the region of the Orion nebula T-association. V0545 Ori |In the region of the Orion nebula T-association. V0546 Ori |In the region of the Orion nebula T-association. V0547 Ori |In the region of the Orion nebula T-association. V0548 Ori |In the region of the open cluster lambda Ori. V0549 Ori |In the region of the open cluster lambda Ori. V0550 Ori |In the region of the Orion nebula T-association. V0551 Ori |In the region of the Orion nebula T-association. V0552 Ori |In the region of the Orion nebula T-association. V0553 Ori |In the region of the Orion nebula T-association. V0554 Ori |In the region of the Orion nebula T-association. V0555 Ori |In the region of the Orion nebula T-association. V0556 Ori |In the region of the Orion nebula T-association. V0557 Ori |In the region of the Orion nebula T-association. V0559 Ori |In the region of the Orion nebula T-association. V0560 Ori |In the region of the Orion nebula T-association. V0561 Ori |In the region of the Orion nebula T-association. V0562 Ori |In the region of the Orion nebula T-association. V0563 Ori |In the region of the Orion nebula T-association. V0564 Ori |In the region of the Orion nebula T-association. V0565 Ori |In the region of the Orion nebula T-association. V0566 Ori |In the region of the Orion nebula T-association. V0567 Ori |In the region of the Orion nebula T-association. V0568 Ori |In the region of the Orion nebula T-association. V0569 Ori |In the region of the Orion nebula T-association. V0570 Ori |In the region of the Orion nebula T-association. V0571 Ori |In the region of the Orion nebula T-association. V0572 Ori |In the region of the open cluster lambda Ori. V0573 Ori |In the region of the Orion nebula T-association. V0574 Ori |In the region of the Orion nebula T-association. V0575 Ori |In the region of the Orion nebula T-association. V0576 Ori |In the region of the Orion nebula T-association. V0577 Ori |In the region of the Orion nebula T-association. V0578 Ori |In the region of the Orion nebula T-association. V0579 Ori |In the region of the Orion nebula T-association. V0580 Ori |In the region of the Orion nebula T-association. V0581 Ori |In the region of the Orion nebula T-association. V0582 Ori |In the region of the Orion nebula T-association. V0584 Ori |In the region of the Orion nebula T-association. V0585 Ori |In the region of the Orion nebula T-association. V0586 Ori |In the region of the Orion nebula T-association. V0587 Ori |In the region of the Orion nebula T-association. V0588 Ori |In the region of the Orion nebula T-association. V0589 Ori |In the region of the Orion nebula T-association. V0590 Ori |In the region of the Orion nebula T-association. V0591 Ori |In the region of the Orion nebula T-association. V0592 Ori |In the region of the Orion nebula T-association. V0593 Ori |In the region of the Orion nebula T-association. V0594 Ori |In the region of the Orion nebula T-association. V0595 Ori |In the region of the nebula IC 434. V0596 Ori |In the region of the open cluster lambda Ori. V0597 Ori |In the region of the nebula IC 434. V0598 Ori |In the region of the open cluster lambda Ori. V0599 Ori |In the region of the Orion nebula T-association. V0600 Ori |In the region of the nebula IC 434. V0601 Ori |In the region of the nebula IC 434. V0602 Ori |In the region of the nebula IC 434. V0603 Ori |In the region of the nebula IC 434. V0604 Ori |In the region of the nebula IC 434. V0605 Ori |In the region of the nebula IC 434. V0606 Ori |In the region of the nebula IC 434. V0607 Ori |In the region of the nebula IC 434. V0608 Ori |In the region of the nebula IC 434. V0610 Ori |In the region of the nebula IC 434. V0611 Ori |In the region of the nebula IC 434. V0612 Ori |VB, SE-comp.; NW-comp.=NSV 02555. In the region of the V0612 Ori |nebula IC 434. V0614 Ori |In the region of T-association FU Ori. V0615 Ori |In the region of the nebula IC 434. V0616 Ori |In the region of the nebula IC 434. V0617 Ori |In the region of the nebula IC 434. V0618 Ori |In the region of the nebula IC 434. V0619 Ori |In the region of the nebula IC 434. V0620 Ori |In the region of the nebula IC 434. V0621 Ori |In the region of the nebula IC 434. V0622 Ori |In the region of the nebula IC 434. V0623 Ori |In the region of the nebula IC 434. V0625 Ori |In the region of T-association FU Ori. V0626 Ori |In the region of T-association FU Ori. V0627 Ori |In the region of T-association FU Ori. V0628 Ori |In the region of T-association FU Ori. V0629 Ori |In the region of T-association FU Ori. V0630 Ori |In the region of T-association FU Ori. V0631 Ori |In the region of T-association FU Ori. V0632 Ori |In the region of T-association FU Ori. V0634 Ori |In the region of T-association FU Ori. V0635 Ori |In the region of T-association FU Ori. V0636 Ori |In the region of T-association FU Ori. V0637 Ori |In the region of T-association FU Ori. V0638 Ori |In the region of T-association FU Ori. V0639 Ori |In the region of T-association FU Ori. V0640 Ori |d <= 0.02P. V0641 Ori |Min II 14.5. V0642 Ori |d = 0.05P?. V0643 Ori |P = 26.2075d? V0647 Ori |Min II 11.9. P var. Min I = 2418005.035 + 0.977575d*E V0647 Ori |(JD2414660 - 23230); since JD2423230 - see Table. V0648 Ori |Min II 12.2. V0649 Ori |In the T-association CO - Ori. VB A (B 15m, 2", 0deg). V0650 Ori |In the region of the open cluster lambda Ori. V0652 Ori |In the region of the Orion nebula T-association. V0654 Ori |In the region of the Orion nebula T-association. V0655 Ori |In the region of the Orion nebula T-association. V0656 Ori |In the region of the Orion nebula T-association. V0657 Ori |In the region of the Orion nebula T-association. V0658 Ori |In the region of the Orion nebula T-association. V0659 Ori |In the region of the Orion nebula T-association. V0667 Ori |Min II 15.0. V0676 Ori |In the region of the Orion nebula T-association. V0677 Ori |In the region of the Orion nebula T-association. V0678 Ori |In the region of the Orion nebula T-association. V0679 Ori |In the region of the Orion nebula T-association. V0680 Ori |In the region of the Orion nebula T-association. V0681 Ori |In the region of the Orion nebula T-association. V0682 Ori |In the region of the Orion nebula T-association. V0683 Ori |In the region of the Orion nebula T-association. V0684 Ori |In the region of the Orion nebula T-association. V0685 Ori |In the region of the Orion nebula T-association. V0685 Ori |A(U) = 1.0m. V0686 Ori |In the region of the Orion nebula T-association. V0687 Ori |In the region of the Orion nebula T-association. V0688 Ori |In the region of the Orion nebula T-association. V0689 Ori |In the region of the Orion nebula T-association. V0690 Ori |In the region of the Orion nebula T-association. V0691 Ori |In the region of the Orion nebula T-association. V0692 Ori |In the region of the Orion nebula T-association. V0693 Ori |In the region of the Orion nebula T-association. V0694 Ori |In the region of the Orion nebula T-association. V0695 Ori |In the region of the Orion nebula T-association. V0696 Ori |In the region of the Orion nebula T-association. V0697 Ori |In the region of the Orion nebula T-association. V0698 Ori |In the region of the Orion nebula T-association. V0699 Ori |In the region of the Orion nebula T-association. V0700 Ori |In the region of the Orion nebula T-association. V0701 Ori |In the region of the Orion nebula T-association. V0702 Ori |In the region of the Orion nebula T-association. V0703 Ori |In the region of the Orion nebula T-association. V0704 Ori |In the region of the Orion nebula T-association. V0705 Ori |In the region of the Orion nebula T-association. V0706 Ori |In the region of the Orion nebula T-association. V0707 Ori |In the region of the Orion nebula T-association. V0708 Ori |In the region of the Orion nebula T-association. V0709 Ori |In the region of the Orion nebula T-association. V0710 Ori |In the region of the Orion nebula T-association. V0711 Ori |In the region of the Orion nebula T-association. V0712 Ori |In the region of the Orion nebula T-association. V0713 Ori |In the region of the Orion nebula T-association. V0713 Ori |A(U) = 4.0m. V0714 Ori |In the region of the Orion nebula T-association. V0715 Ori |In the region of the Orion nebula T-association. V0716 Ori |In the region of the Orion nebula T-association. V0717 Ori |In the region of the Orion nebula T-association. V0718 Ori |In the region of the Orion nebula T-association. V0718 Ori |Probably the sf-component of a very close pair. V0719 Ori |In the region of the Orion nebula T-association. V0720 Ori |In the region of the Orion nebula T-association. V0721 Ori |In the region of the Orion nebula T-association. V0722 Ori |In the region of the Orion nebula T-association. V0723 Ori |In the region of the Orion nebula T-association. V0724 Ori |In the region of the Orion nebula T-association. V0725 Ori |In the region of the Orion nebula T-association. V0726 Ori |In the region of the Orion nebula T-association. V0727 Ori |In the region of the Orion nebula T-association. V0728 Ori |In the region of the Orion nebula T-association. V0729 Ori |In the region of the Orion nebula T-association. V0730 Ori |In the region of the Orion nebula T-association. V0731 Ori |In the region of the Orion nebula T-association. V0732 Ori |In the region of the Orion nebula T-association. V0733 Ori |In the region of the Orion nebula T-association. V0734 Ori |In the region of the Orion nebula T-association. V0735 Ori |In the region of the Orion nebula T-association. V0736 Ori |In the region of the Orion nebula T-association. V0737 Ori |In the region of the Orion nebula T-association. V0737 Ori |A(U) > 2.4m. V0738 Ori |In the region of the Orion nebula T-association. V0739 Ori |In the region of the Orion nebula T-association. V0740 Ori |In the region of the Orion nebula T-association. V0740 Ori |A(pg) > 4.0m. V0741 Ori |In the region of the Orion nebula T-association. V0742 Ori |In the region of the Orion nebula T-association. V0744 Ori |In the region of the Orion nebula T-association. V0745 Ori |In the region of the Orion nebula T-association. V0746 Ori |In the region of the Orion nebula T-association. V0747 Ori |In the region of the Orion nebula T-association. V0748 Ori |In the region of the Orion nebula T-association. V0749 Ori |In the region of the Orion nebula T-association. V0750 Ori |In the region of the Orion nebula T-association. V0751 Ori |In the region of the Orion nebula T-association. V0752 Ori |In the region of the Orion nebula T-association. V0753 Ori |In the region of the Orion nebula T-association. V0754 Ori |In the region of the Orion nebula T-association. V0755 Ori |In the region of the Orion nebula T-association. V0756 Ori |In the region of the Orion nebula T-association. V0757 Ori |In the region of the Orion nebula T-association. V0758 Ori |In the region of the Orion nebula T-association. V0759 Ori |In the region of the Orion nebula T-association. V0760 Ori |In the region of the Orion nebula T-association. V0761 Ori |In the region of the Orion nebula T-association. V0762 Ori |In the region of the Orion nebula T-association. V0763 Ori |In the region of the Orion nebula T-association. V0764 Ori |In the region of the Orion nebula T-association. V0765 Ori |In the region of the Orion nebula T-association. V0766 Ori |In the region of the Orion nebula T-association. V0767 Ori |In the region of the Orion nebula T-association. V0767 Ori |A(U) = 1.5m. V0768 Ori |In the region of the Orion nebula T-association. V0770 Ori |In the region of the Orion nebula T-association. V0771 Ori |In the region of the Orion nebula T-association. V0772 Ori |In the region of the Orion nebula T-association. V0773 Ori |In the region of the Orion nebula T-association. V0774 Ori |In the region of the Orion nebula T-association. V0775 Ori |In the region of the Orion nebula T-association. V0776 Ori |In the region of the Orion nebula T-association. V0777 Ori |In the region of the Orion nebula T-association. V0778 Ori |In the region of the Orion nebula T-association. V0778 Ori |A(pg) = 1.6m. V0779 Ori |In the region of the Orion nebula T-association. V0780 Ori |In the region of the Orion nebula T-association. V0780 Ori |A(U) = 1.0m. V0781 Ori |In the region of the Orion nebula T-association. V0782 Ori |In the region of the Orion nebula T-association. V0783 Ori |In the region of the Orion nebula T-association. V0783 Ori |A(pg) = 3.0m. V0784 Ori |In the region of the Orion nebula T-association. V0785 Ori |In the region of the Orion nebula T-association. V0786 Ori |In the region of the Orion nebula T-association. V0787 Ori |In the region of the Orion nebula T-association. V0788 Ori |In the region of the Orion nebula T-association. V0789 Ori |In the region of the Orion nebula T-association. V0790 Ori |In the region of the Orion nebula T-association. V0791 Ori |In the region of the Orion nebula T-association. V0792 Ori |In the region of the Orion nebula T-association. V0793 Ori |In the region of the Orion nebula T-association. V0794 Ori |In the region of the Orion nebula T-association. V0795 Ori |In the region of the Orion nebula T-association. V0796 Ori |In the region of the Orion nebula T-association. V0797 Ori |In the region of the Orion nebula T-association. V0798 Ori |In the region of the Orion nebula T-association. V0799 Ori |In the region of the Orion nebula T-association. V0800 Ori |In the region of the Orion nebula T-association. V0801 Ori |In the region of the Orion nebula T-association. V0802 Ori |In the region of the Orion nebula T-association. V0803 Ori |In the region of the Orion nebula T-association. V0804 Ori |In the region of the Orion nebula T-association. V0805 Ori |In the region of the Orion nebula T-association. V0806 Ori |In the region of the Orion nebula T-association. V0807 Ori |In the region of the Orion nebula T-association. V0808 Ori |In the region of the Orion nebula T-association. V0810 Ori |In the region of the Orion nebula T-association. V0811 Ori |In the region of the Orion nebula T-association. V0812 Ori |In the region of the Orion nebula T-association. V0813 Ori |In the region of the Orion nebula T-association. V0814 Ori |In the region of the Orion nebula T-association. V0815 Ori |In the region of the Orion nebula T-association. V0816 Ori |In the region of the Orion nebula T-association. V0817 Ori |In the region of the Orion nebula T-association. V0818 Ori |In the region of the Orion nebula T-association. V0819 Ori |In the region of the Orion nebula T-association. V0820 Ori |In the region of the Orion nebula T-association. V0821 Ori |In the region of the Orion nebula T-association. V0822 Ori |In the region of the Orion nebula T-association. V0823 Ori |In the region of the Orion nebula T-association. V0824 Ori |In the region of the Orion nebula T-association. V0825 Ori |In the region of the Orion nebula T-association. V0826 Ori |In the region of the Orion nebula T-association. V0827 Ori |In the region of the Orion nebula T-association. V0828 Ori |In the region of the Orion nebula T-association. V0829 Ori |In the region of the Orion nebula T-association. V0830 Ori |In the region of the Orion nebula T-association. V0831 Ori |In the region of the Orion nebula T-association. V0832 Ori |In the region of the Orion nebula T-association. V0833 Ori |In the region of the Orion nebula T-association. V0834 Ori |In the region of the Orion nebula T-association. V0835 Ori |In the region of the Orion nebula T-association. V0836 Ori |In the region of the Orion nebula T-association. V0836 Ori |A(U) > 1.5m. V0837 Ori |In the region of the Orion nebula T-association. V0838 Ori |In the region of tbe Orion nebula T-association. V0839 Ori |In the region of tbe Orion nebula T-association. V0840 Ori |In the region of the Orion nebula T-association. V0840 Ori |A(pg) = 0.7m. V0841 Ori |In the region of the Orion nebula T-association. V0842 Ori |In the region of the Orion nebula T-association. V0843 Ori |In the region of the Orion nebula T-association. V0844 Ori |In the region of the Orion nebula T-association. V0845 Ori |In the region of the Orion nebula T-association. V0846 Ori |In the region of the Orion nebula T-association. V0847 Ori |In the region of the Orion nebula T-association. V0848 Ori |In the region of the Orion nebula T-association. V0849 Ori |In the region of the Orion nebula T-association. V0850 Ori |In the region of the Orion nebula T-association. V0851 Ori |In the region of the Orion nebula T-association. V0852 Ori |In the region of the Orion nebula T-association. V0853 Ori |In the region of the Orion nebula T-association. V0854 Ori |In the region of the Orion nebula T-association. V0855 Ori |In the region of the Orion nebula T-association. V0855 Ori |A(U) > 2.0m. V0856 Ori |In the region of the Orion nebula T-association. V0857 Ori |In the region of the Orion nebula T-association. V0857 Ori |A(pg) > 5.0m. V0858 Ori |In the region of the Orion nebula T-association. V0859 Ori |In the region of the Orion nebula T-association. V0860 Ori |In the region of the Orion nebula T-association. V0861 Ori |In the region of the Orion nebula T-association. V0862 Ori |In the region of the Orion nebula T-association. V0863 Ori |In the region of the Orion nebula T-association. V0864 Ori |In the region of the Orion nebula T-association. V0865 Ori |In the region of the Orion nebula T-association. V0866 Ori |In the region of the Orion nebula T-association. V0867 Ori |In the region of the Orion nebula T-association. V0867 Ori |A(pg)>3.0m. V0868 Ori |In the region of the Orion nebula T-association. V0869 Ori |In the region of the Orion nebula T-association. V0870 Ori |In the region of the Orion nebula T-association. V0871 Ori |In the region of the Orion nebula T-association. V0872 Ori |In the region of the Orion nebula T-association. V0873 Ori |In the region of the Orion nebula T-association. V0874 Ori |In the region of the Orion nebula T-association. V0875 Ori |In the region of the Orion nebula T-association. V0876 Ori |In the region of the Orion nebula T-association. V0876 Ori |Southem component of a close pair. V0877 Ori |In the region of the Orion nebula T-association. V0878 Ori |In the region of the Orion nebula T-association. V0879 Ori |In the region of the Orion nebula T-association. V0880 Ori |In the region of the Orion nebula T-association. V0881 Ori |In the region of the Orion nebula T-association. V0882 Ori |In the region of the Orion nebula T-association. V0883 Ori |In the region of the Orion nebula T-association. V0883 Ori |In the apex of a cometary nebula. V0884 Ori |In the region of the Orion nebula T-association. V0885 Ori |In the region of the Orion nebula T-association. V0886 Ori |In the region of the Orion nebula T-association. V0886 Ori |A(pg) > 3.5m. V0888 Ori |In the region of the Orion nebula T-association. V0889 Ori |In the region of the Orion nebula T-association. V0890 Ori |In the region of the Orion nebula T-association. V0891 Ori |In the region of the Orion nebula T-association. V0892 Ori |In the region of the Orion nebula T-association. V0892 Ori |Southern component of a pair (ro = 3"). V0893 Ori |In the region of the Orion nebula T-association. V0893 Ori |A(U) = 2.0m. V0894 Ori |In the region of the Orion nebula T-association. V0895 Ori |In the region of the Orion nebula T-association. V0896 Ori |In the region of the Orion nebula T-association. V0897 Ori |In the region of the Orion nebula T-association. V0898 Ori |In the region of the Orion nebula T-association. V0899 Ori |In the region of the Orion nebula T-association. V0900 Ori |In the region of the Orion nebula T-association. V0900 Ori |A(pg) > 2.5m. V0901 Ori |In the region of the nebula IC 434. V0902 Ori |In the region of the Orion nebula T-association. V0904 Ori |In the region of the Orion nebula T-association. V0905 Ori |In the region of the Orion nebula T-association. V0906 Ori |In the region of the Orion nebula T-association. V0907 Ori |In the region of the Orion nebula T-association. V0908 Ori |In the region of the Orion nebula T-association. V0909 Ori |In the region of the Orion nebula T-association. V0916 Ori |P = 0.28297d? Member of the open cluster NGC 2169. V0917 Ori |Member of the open cluster NGC 2169. V0918 Ori |In the region of the Orion nebula T-association. V0919 Ori |In the region of the Orion nebula T-association. V0920 Ori |In the region of the Orion nebula T-association. V0921 Ori |In the region of the Orion nebula T-association. V0922 Ori |In the region of the Orion nebula T-association. V0923 Ori |In the region of the Orion nebula T-association. V0924 Ori |In the region of the Orion nebula T-association. V0926 Ori |In the region of the Orion nebula T-association. V0927 Ori |In the region of the Orion nebula T-association. V0928 Ori |In the region of the Orion nebula T-association. V0929 Ori |In the region of the Orion nebula T-association. V0930 Ori |In the region of the Orion nebula T-association. V0931 Ori |In the region of the Orion nebula T-association. V0932 Ori |In the region of the Orion nebula T-association. V0933 Ori |In the region of the Orion nebula T-association. V0934 Ori |In the region of the Orion nebula T-association. V0935 Ori |In the region of the Orion nebula T-association. V0937 Ori |In the region of the Orion nebula T-association. V0938 Ori |In the region of the Orion nebula T-association. V0939 Ori |In the region of the Orion nebula T-association. V0941 Ori |In the region of the Orion nebula T-association. V0942 Ori |In the region of the Orion nebula T-association. V0943 Ori |In the region of the Orion nebula T-association. V0945 Ori |In the region of the Orion nebula T-association. V0946 Ori |In the region of the Orion nebula T-association. V0947 Ori |In the region of the Orion nebula T-association. V0948 Ori |In the region of the Orion nebula T-association. V0949 Ori |In the region of the Orion nebula T-association. V0950 Ori |In the region of the Orion nebula T-association. V0951 Ori |In the region of the Orion nebula T-association. V0952 Ori |In the region of the Orion nebula T-association. V0953 Ori |In the region of the nebula IC 434. V0956 Ori |In the region of the nebula IC 434. V0957 Ori |In the region of the nebula IC 434. V0958 Ori |In the region of the Orion nebula T-association. V0960 Ori |In the region of the nebula IC 434. V0961 Ori |In the region of the Orion nebula T-association. V0964 Ori |P var. Max = 2415800.389 + 0.5046772d*E V0964 Ori |(JD2415800 - 21010); Max = 2424500.446 + 0.50466477d*E V0964 Ori |(JD2424500 - 30500); since JD2431500 - see Table. V0966 Ori |In the region of the Orion nebula T-association. V0967 Ori |In the region of the Orion nebula T-association. V0968 Ori |In the region of the Orion nebula T-association. V0969 Ori |In the region of the Orion nebula T-association. V0970 Ori |In the region of the Orion nebula T-association. V0971 Ori |In the region of the Orion nebula T-association. V0972 Ori |In the region of the Orion nebula T-association. V0973 Ori |In the region of the Orion nebula T-association. V0974 Ori |In the region of the Orion nebula T-association. V0975 Ori |In the region of the Orion nebula T-association. V0976 Ori |In the region of the Orion nebula T-association. V0977 Ori |In the region of the Orion nebula T-association. V0978 Ori |In the region of the Orion nebula T-association. V0979 Ori |In the region of the Orion nebula T-association. V0980 Ori |In the region of the Orion nebula T-association. V0981 Ori |In the region of the Orion nebula T-association. V0982 Ori |In the region of the Orion nebula T-association. V0983 Ori |In the region of the Orion nebula T-association. V0984 Ori |In the region of the Orion nebula T-association. V0985 Ori |In the region of the Orion nebula T-association. V0986 Ori |In the region of the Orion nebula T-association. V0987 Ori |In the region of the Orion nebula T-association. V0988 Ori |In the region of the Orion nebula T-association. V0989 Ori |In the region of the Orion nebula T-association. V0990 Ori |In the region of the Orion nebula T-association. V0991 Ori |In the region of the Orion nebula T-association. V0992 Ori |In the region of the Orion nebula T-association. V0994 Ori |In the region of the Orion nebula T-association. V0995 Ori |In the region of the Orion nebula T-association. V0996 Ori |In the region of the Orion nebula T-association. V0997 Ori |In the region of the Orion nebula T-association. V0998 Ori |mu = 0.28", ro = 221deg. V0999 Ori |In the region of the Orion nebula T-association. V1000 Ori |In the region of the Orion nebula T-association. V1001 Ori |In the region of the Orion nebula T-association. V1002 Ori |In the region of the Orion nebula T-association. V1003 Ori |mu = 0.272", ro = 60.8deg. V1004 Ori |VB A (B 10.57m, 37", 204deg); SB (P = 2.74d). V1005 Ori |The range of light variations (characteristic for BY Dra V1005 Ori |type variability) between the flares is given in the Table; V1005 Ori |the amplitude of the flares A(U) can reach 3.2m. V1006 Ori |In the region of the Orion nebula T-association. V1007 Ori |In the region of the Orion nebula T-association. V1016 Ori |In the region of the Orion nebula T-association. V1016 Ori |In the cluster NGC 1976. Orion Trapezium V1016 Ori |member: teta1 Ori A (B = BM Ori, 8.7", 32deg; C 5.13m, V1016 Ori |13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.001P. V1017 Ori |In the region of the Orion nebula T-association. V1018 Ori |In the region of the Orion nebula T-association. V1019 Ori |In the region of the Orion nebula T-association. V1020 Ori |In the region of the Orion nebula T-association. V1022 Ori |In the region of T-association FU Ori. V1028 Ori |P = 6d? V1029 Ori |In the region of the Orion nebula T-association. V1030 Ori |In the region of the nebula IC 434. (sig Ori) E V1030 Ori |(A 4.1m; B 5.1m, A = 0.247", P = 170yr; C 8.79m, 11.2", V1030 Ori |238deg; D 6.66m, 12.9", 84deg; E 41.6", 61deg). Min I V1030 Ori |(HeI) = 2442802.48 + 1.19080d*E. Unusual helium variable. V1030 Ori |Epoch of Min I brightness is given in the Table V1030 Ori |(Min II 6.71, Min II - Min I = 0.43P). This epoch is being V1030 Ori |observed by 0.18P later than the epoch of minimum strength V1030 Ori |of the HeI lambda 4026 A line. According to [09524], light V1030 Ori |minima are due to "eclipses" of the star surface V1030 Ori |by two isolated clouds (consisting of hydrogen and V1030 Ori |helium), which are located almost oppositely near V1030 Ori |the intersections of the magnetic And rotational V1030 Ori |equator. V1031 Ori |VB (0.159", 104deg, 1980.7). Min II 6.32; DII = 0.017P. V1034 Ori |Epoch of light minimum is given. V1035 Ori |In the region of the Orion nebula T-association. V1036 Ori |In the region of the Orion nebula T-association. V1037 Ori |In the region of the Orion nebula T-association. V1038 Ori |In the region of the Orion nebula T-association. V1039 Ori |In the region of the Orion nebula T-association. V1040 Ori |In the region of the Orion nebula T-association. V1041 Ori |In the region of the Orion nebula T-association. V1042 Ori |In the region of the Orion nebula T-association. V1043 Ori |In the region of the Orion nebula T-association. V1044 Ori |In the region of the Orion nebula T-association. V1045 Ori |In the region of the Orion nebula T-association. V1046 Ori |In the region of the Orion nebula T-association. V1046 Ori |SB 1. Min II 6.58. Possibly an ellipsoidal variable, its V1046 Ori |light variations being superimposed by light variations of V1046 Ori |the primary component of SX Ari type: V1046 Ori |Min (HeI) = 2442812.23 + 0.9015d*E [08054]. V1047 Ori |In the region of the Orion nebula T-association. V1048 Ori |In the region of the Orion nebula T-association. V1049 Ori |In the region of the Orion nebula T-association. V1050 Ori |In the region of the Orion nebula T-association. V1052 Ori |In the region of the Orion nebula T-association. V1053 Ori |In the region of the Orion nebula T-association. V1054 Ori |Epoch of light minimum is given. P = 8.596d?, P = 8.674d? V1055 Ori |P(X) = 5.2d [09528]. V1056 Ori |VB A (B 9.8m, 28.7", 58deg). V1058 Ori |In the region of the Orion nebula T-association. V1059 Ori |In the region of the Orion nebula T-association. V1060 Ori |In the region of the Orion nebula T-association. V1061 Ori |In the region of the Orion nebula T-association. V1062 Ori |In the region of the Orion nebula T-association. V1063 Ori |In the region of the Orion nebula T-association. V1064 Ori |In the region of the Orion nebula T-association. V1065 Ori |In the region of the Orion nebula T-association. V1066 Ori |In the region of the Orion nebula T-association. V1067 Ori |In the region of the Orion nebula T-association. V1068 Ori |In the region of the Orion nebula T-association. V1069 Ori |In the region of the Orion nebula T-association. V1070 Ori |In the region of the Orion nebula T-association. V1071 Ori |In the region of the Orion nebula T-association. V1072 Ori |In the region of the Orion nebula T-association. V1073 Ori |In the region of the Orion nebula T-association. V1074 Ori |In the region of the Orion nebula T-association. V1075 Ori |In the region of the Orion nebula T-association. V1076 Ori |In the region of the Orion nebula T-association. V1077 Ori |In the region of the Orion nebula T-association. V1078 Ori |In the region of the Orion nebula T-association. V1079 Ori |In the region of the Orion nebula T-association. V1080 Ori |In the region of the Orion nebula T-association. V1081 Ori |In the region of the Orion nebula T-association. V1082 Ori |In the region of the Orion nebula T-association. V1083 Ori |In the region of the Orion nebula T-association. V1084 Ori |In the region of the Orion nebula T-association. V1377 Ori |SB?, Porb ~ 5.5 to 6.5d. V1380 Ori |In a bright nebula. alf Ori |VB A (B 14.5m, 39.8", 110deg). Min = 2410600 + 2070d*E alf Ori |(1840 - 1929) [01012]. Since 1929 - see Table. alf Ori |The main variation is superimposed by the waves alf Ori |with P = 200 - 400d. Dust-gaseous shell (r = 50") alf Ori |[09529]. del Ori |VB A (A 0.217", 144deg, 1980; B 14.0m, 33.1", 227deg; del Ori |C 6.84m, 53.5", 359deg). Orion Belt cluster member. del Ori |Min II 2.20. del Ori |Apsidal motion (P = 210 yr). Shape of the light curve del Ori |varies. The intrinsic brightness variability of the del Ori |components is possible. eps Ori |Orion Belt cluster member. eta Ori |VB Aab (AC 0.037", 111deg, 1979.0, P = 9.219 yr [09535]; eta Ori |B 4.8m, 1.60", 76deg, 1976.0; C 9.4m, 115", 51deg). EA/DM. eta Ori |Min II 3.57. The range of combined light variation of the eta Ori |components AAb (SB 2, P = 7.989268d), AC, and B is given eta Ori |in the Table. Outside eclipses there are sinusoidal light eta Ori |variations of the system with A(V) = 0.05m due to eta Ori |pulsations of the component Ab [09535] with P = 0.30197d eta Ori |[09536] or 0.30145d [09537]. According to [08566] these eta Ori |variations were not observed between 1970 and 1976. pi 5 Ori |Min II 3.73. The period is improved using radial pi 5 Ori |velocities [04627]. psi Ori |VB A (B 11.1m, 2.7", 323deg; C 13.88m, 83", 196deg). psi Ori |Min II 4.58. The period is determined on the base of psi Ori |radial velocities [09541]. R Pav |Pvar. Max = 2411219 + 228.34d (JD2411000 - 18500); R Pav |Max = 2418527 + 230.95d*E (JD2418500 - 30000); R Pav |since JD2430000 - see Table. S Pav |P var. Max = 2421479 + 389.64d*E(JD2421000 - 31000); S Pav |since JD2431000 - see Table. Delta(m) var strongly. S Pav |Min II is sometimes observed after Max I. T Pav |P var. Max = 2413328 + 243.45d*E(JD2405700 - T Pav |25500); Max = 2425499 + 245.11d*E(JD2425500 - T Pav |32500); since JD2432500 - see Table. V Pav |VBA (B 14.0m vis, 15", 327deg). Mean brightness var, V Pav |P2 = 3735d, 9.7m - 10.7m. W Pav |P var. Before JD2431000 Max = 2413778 + 282.92d*E; W Pav |since JD2431000 - see Table. RT Pav |Mean light var, 10.4m - 11.1m 1649, P2 = 757d. SU Pav |P var. Max = 2430036 + 245.18d*E (JD2411000 - 30100) SU Pav |[00001]; during JD247700 - 40000 - see Table. SX Pav |mu alpha = +0.0166s, mu delta = -0.05". TW Pav |Before JD2420400 Max = 2417760 + 397.d*E. YY Pav |Delta(m) var strongly. P possibly is twice longer, in that YY Pav |case Min II 14.4. AR Pav |Depth of eclipses Delta(m) = 2m B, d = 0.05P. Expanding AR Pav |shell. BD Pav |Only one outburst was observed [00629]. Brightness BD Pav |flickering. Eclipses according to the elements BD Pav |Min I = 2444412.676 + 0.1793015d*E, Delta(m) ~0.5m [09191]. BD Pav |Outside outburst, 15.40m - 16.21m. BF Pav |Min II 11.9. BI Pav |Min II (Delta(m) ~0.05m) is possible. DF Pav |Epoch of min is given. Light curve shape strongly var. DN Pav |Delta(S) = 8:. DW Pav |Min II 16.3. EG Pav |Twice shorter P is possible [00001]. EL Pav |Min II 15.5. EN Pav |Elements need confirmation. EQ Pav |Red. FY Pav |Min II? JD2436784.37. HL Pav |Blazhko effect? HP Pav |Min II 15.5. HQ Pav |Min II 12.7. HY Pav |Min II 12.1. IL Pav |RRC type is possible. KR Pav |Min II 14.1. KZ Pav |VB A (B 8.7m, 6.7", 119deg, 1971; C 9.2m, BC 1.0", 329deg, KZ Pav |1971). P var. Min = 2430448.617 + 0.949880d*E KZ Pav |(JD2416000 - 30000) [00001]; since JD2430000 - see Table. KZ Pav |Min II is present. LL Pav |Min II 15.1. LO Pav |Min II 16.5. LR Pav |Min II 15.3. LT Pav |Min II 12.2. LV Pav |Min II 14.3. LY Pav |Min II 14.9. MQ Pav |Epoch of Min is given. EW/KW type with twice longer P is MQ Pav |possible. MR Pav |Possible elements Max = 2436731.40 + 0.3737d*E [00001]. MS Pav |Min II 14.1. MW Pav |d = 0.08P. Min II 8.92, dII = 0.11P. NP Pav |Deep Min II. NW Pav |[A/H] = -0.7. OY Pav |The chart in [06286] is wrong. V0382 Pav |Type EW: is also possible. kap Pav |P var. Max = 2419619.38 + 9.0898d*E (JD2411930 - 22550); kap Pav |Max = 2425987.12 + 9.1028d*E (JD2422550 - 26980); kap Pav |Max = 2430530.67 + 9.0833d*E (JD2426980 - 31345); kap Pav |Max = 2433239.87 + 9.0956d*E (JD2431345 - 34045); kap Pav |Max = 2434693.11 + 9.0653d*E (JD2434045 - 37000); kap Pav |since JD2440000 - see Table. [Fe/H] = 0.0/ - 0.4. kap Pav |Moderately high Z coordinate (IZI ~240 pc provided kap Pav |the period - luminosity relation for DCEP stars is valid), kap Pav |low radial velocity. The period is not typical kap Pav |for CW stars. Ca II emission was noticed in the spectrum. lam Pav |VB A (B 12.4m, 63.1", 206deg). rho Pav |The main light variation P1 (see Table) with a rho Pav |semiamplitude delta(y) = 0.0069m is superposed by rho Pav |oscillations with P2 = 0.1131d (delta(y) = 0.0031m), rho Pav |P3 = 0.1612d (delta(y) = 0.0029m). R Peg |OH, H2O, SiO maser. P var. Max = 2396327 + 381.9d*E R Peg |(JD2396300 - 2408200); Max = 2413012 + 371.4d*E R Peg |(JD2413000 - 19800); Max = 2420092 + 379.77d*E R Peg |(JD2420000 - 31100) [00960]; since JD2431100 - see Table. T Peg |P var. Max = 2398452 + 371.0d*E (JD2398400 - 2408900); T Peg |Max = 2413697 + 386.8d*E (JD2413600 - 18700); T Peg |Max = 2421016 + 362.5d*E (JD2420900 - 28000) [00960]; T Peg |Max = 2434343 + 376.0d*E (JD2428300 - 34300); T Peg |Max = 2440984 + 368.7d*E (JD2434300 - 41000); T Peg |since JD2441000 - see Table. U Peg |Min II 9.73. P var. U Peg |There is a square term in the elements: U Peg |-2.468D*10**(-11)*E**2. U Peg |0 - C = 0.00323d*sin((2pi/16330)E + 0.418pi). Shape of U Peg |the light curve varies. W Peg |SiO maser. P var. Max = 2413819 + 343.2d*E W Peg |(JD2413800 - 26600); Max = 2427162 + 345.5d*E W Peg |(JD2426600 - 32100) [00960]; Max = 2439690 + 348.75d*E W Peg |(JD2432300 - 39700) [00001]; since JD2441400 - see Table. X Peg |P var. Max = 2414713 + 200.3d*E (JD2414700 - 21300); X Peg |Max = 2420105 + 204.3d*E (JD2420100 - 23800); X Peg |Max = 2423570 + 199.8d*E (JD2423600 - 31000) [00960]; X Peg |Max = 2432006 + 208d*E (JD2431000 - 32100); X Peg |Max = 2434206 + 200.0d*E (JD2432100 - 39300); X Peg |since JD2438400 - see Table. Z Peg |P var. Max = 2415433 + 318.9d*E (JD2398800 - 2420550); Z Peg |Max = 2420207 + 328.0d*E (JD2420200 - 32000) [00960]; Z Peg |Max = 2432005 + 325.8d*E (JD2432000 - 37900); Z Peg |Max = 2437870 + 319d*E (JD2437500 - 40100); Z Peg |Max = 2442086 + 328.0d*E (JD2440100 - 43100); Z Peg |since JD2442100 - see Table. RR Peg |P var. Max = 2417582 + 268.3d*E (JD2416700 - 17850) RR Peg |[00001]; Max = 2417859 + 260.8d*E (JD2417850 - 21000) RR Peg |[00960]; since JD2421000 - see Table. RS Peg |P var. Max = 2415846 + 431.5d*E (JD2415800 - 18450); RS Peg |Max = 2418434 + 404.1d*E (JD2418400 - 24200); RS Peg |Max = 2424514 + 413.4d*E (JD2424500 - 34900) [00960]; RS Peg |Max = 2436496 + 403.4d*E (JD2435700 - 38600) [00001]; RS Peg |since JD2438500 - see Table. RT Peg |VB A (B 10.5m, 15.6", 291deg). P var. RT Peg |Max = 2423609 + 215.0d*E (JD2416000 - 24300); RT Peg |Max = 2428149 + 216.6d*E (JD2424300 - 32100); RT Peg |since JD2432100 - see Table. RU Peg |VB A (B 12.5m, 12", 18deg); SB2 (Porb = 0.3746d [09570]). RU Peg |There are also light oscillations with P = 11.6s RU Peg |and 50s [09571]. RV Peg |Emission. Light curve (1907 - 1973) [09572]. P var. RV Peg |Max = 2428735 + 388.4d*E (JD2417000 - 32640); RV Peg |Max = 2430680 + 390.9d*E (JD2430200 - 38900); RV Peg |since JD2438800 - see Table. RW Peg |P var. Max = 2419393 + 208.4d*E (JD2412700 - 19400); RW Peg |Max = 2421520 + 213.0d*E (JD2419390 - 21550); RW Peg |Max = 2427133 + 208.0d*E (JD2421500 - 27150); RW Peg |since JD2427300 - see Table. RX Peg |P2 = 110d:. RY Peg |VB B (A = RZ Peg; B 20", 252deg). RZ Peg |VB A (B = RY Peg:20", 252deg). SC 6/9 - e. P var. RZ Peg |Max = 2423361 + 441.4d*E (JD2411400 - 26450); RZ Peg |Max = 2431215 + 434.0d*E (JD2426400 - 33000); RZ Peg |since JD2433000 - see Table. SS Peg |P var. Max = 2416390 + 410.8d*E (JD2415500 - 20000); SS Peg |Max = 2422235 + 423.8d*E (JD2420000 - 27000); SS Peg |Max = 2427270 + 403.4d*E (JD2427000 - 29000); SS Peg |Max = 2437218 + 416.35d*E (JD2428500 - 43000); SS Peg |since JD2443000 - see Table. SV Peg |H2O emission. SX Peg |S 2.5/6 e. P var. Max = 2436043 + 306.56d*E SX Peg |(JD2414800 - 38300); since JD2438300 - see Table. TU Peg |P var. Max = 2417800 + 320.8d*E (JD2404300 - 18450); TU Peg |Max = 2420730 + 328.4d*E (JD2418450 - 20800); TU Peg |Max = 2428080 + 319.6d*E (JD2420800 - 31600); TU Peg |since JD2432800 - see Table. TW Peg |H2O maser. The basic light variation with the period given TW Peg |in the Table is superimposed by small oscillations TW Peg |with P = 94.13d. TY Peg |Min II 10.2. P var. Min I hel = 2419520.476 + TY Peg |3.0922754d*E (JD2412300 - 19600) [02389]; Min I hel = TY Peg |2425918.348 + 3.092252d*E (JD2419600 - 26000) TY Peg |[00001]; since JD2426000 - see Table. TZ Peg |P var? Max = 2425892 + 213.7d*E (JD2410000 - 28000); TZ Peg |since JD2430000 - see Table. UU Peg |OH, H2O maser. UW Peg |According to [08837] P = 60d. UX Peg |P var. Min = 2428428.386 + 1.544618d*E (JD2422100 - UX Peg |28430) [00230]; Min = 2431273.597 + 1.544632d*E UX Peg |(JD2428420 - 34000) [00001]; since JD2434000 - see Table. VV Peg |Delta(S) = 8. P var. Max = 2420105.296 + 0.48837765d*E VV Peg |(JD2420000 - 28900); Max = 2433217.268 + 0.48838307d*E VV Peg |(JD2432800 - 38000) [03506]; since JD2438000 - see Table. VW Peg |P = 2.341295d? VX Peg |The basic light variation is superimposed by the secondary VX Peg |one with P = 80 - 90d:. VZ Peg |[Fe/H] = -1.75. WW Peg |P var. Max = 2433142 + 371.6d*E (JD2415670 - 33200) WW Peg |[00001]; since JD2436800 - see Table. ZZ Peg |Min II 12.5. AE Peg |P var. Max = 2415470.866 + 0.4967388d*E (JD2415500 - AE Peg |21000); Max = 2426161.544 + 0.496725d*E (JD2425400 - AE Peg |31500); Max = 2432632.809 + 0.496692d*E (JD2431500 - AE Peg |36000) [00001]; during JD2436000 - 40000 - see Table. AE Peg |Delta(S) = 6.3. AG Peg |SB2 (Porb = 820d [09580]). AG Peg |Maximum of brightness was in 1870, then the very AG Peg |slow light decrease was observed that was superimposed AG Peg |since 1935 by periodical light oscillations with AG Peg |A = 0.4m V AG Peg |and P = Porb: Min = 2428250 + 827.d*E ( JD2428000-43000) AG Peg |[09587]. After JD2442300 the period probably has changed: AG Peg |Min = 2442370 + 760d*E [09587]. In 1962 - 1979 the range of AG Peg |brightness was 7.95m - 8.55m V; M - m = 0.50P. AG Peg |Light minima correspond to the epochs of inferior AG Peg |conjunction of M 3 III component. Spectrum var: Beq AG Peg |(1893 - 1919); since 1922 the spectrum is symbiotic one, AG Peg |the M star spectrum being more noticeable. AG Peg |Surrounded by a radio nebula with 1" half-power diameter. AN Peg |P var. Max = 2428045 + 274.1d*E (JD2424500 - 38500) AN Peg |[09581]; since JD2438500 - see Table. AO Peg |Delta(S) = 4.3. AQ Peg |Min II 10.47; d = 0.030P. P var. Min I = 2424749.335 + AQ Peg |5.548419d*E (JD2424000 - 34000) [00980]; AQ Peg |since JD2434000 - see Table. AS Peg |Of the two stars circled in the chart in [06286], the southern AS Peg |component varies. AT Peg |Min II 9.04. P var. Min I = 2425862.337 + 1.1460988d*E AT Peg |(JD2425800 - 37500) [00001]; Min I = 2437497.542 + AT Peg |1.146080d*E (JD2437490 - 40000) [06101]; Min I = AT Peg |2440407*4370 + 1.1461007d*E (JD2440000 - 42400) AT Peg |[00001]; since JD2442400 - see Table. AU Peg |Cepheid in a close binary system. AU Peg |SB1 (Porb = 53.319d, K1 = 41.8 km/s, gamma = -4.1 km/s, AU Peg |E = 0.12 [09582]). [Fe/H] = 0.1. AU Peg |P var. Max = 2428729.76 + 2.3978d*E (JD2426500 - 28750) AU Peg |[00916]; Max = 2433151.976 + 2.38934d*E (JD2433150 - 35800); AU Peg |Max = 2439039.08 + 2.39079d*E (JD2435800 - 39100) [00001]; AU Peg |since JD2441700 - see Table. AU Peg |There is a square term in the elements given in the Table: AU Peg |+2.246d*10**(-6)*E**2. The shape of the light curve varies: AU Peg |0.20P < M - m < 0.47P. AV Peg |P var. Max = 2416347.713 + 0.39036510d*E AV Peg |(JD2414000 - 26500) [00752]; Max = 2426582.301 + AV Peg |0.39037015d*E (JD2426500 - 36000) [09584]; AV Peg |since JD2436000 - see Table. [Fe/H] = +0.02. AW Peg |d = 0.07P, Min II 7.60. BB Peg |Depth of Min II 0.60m. BB Peg |There is a square term in the elements given in the Table: BB Peg |+2.3d*10**(-11)*E**2. dI = 0.05P; dII = 0.00P. BF Peg |P var. Max = 2426589.293 + 0.495796d*E + 2.8d*10**(-9)*E**2 BF Peg |(JD2426500 - 28800) [00522]; Max = 2433200.312 + BF Peg |0.495796d*E (JD2429400 - 33200) [00001]; Max = BF Peg |2437583.343 + 0.495674d*E (JD2437500 - 39400) BF Peg |[00001]; since JD2442650 - see Table. BG Peg |P var. Min = 2427386.3705 + 1.952452d*E (JD2426000 - 35000) BG Peg |[03567]; Min = 2436453.509 + 1.95238d*E (JD2435000 - 43500) BG Peg |[03624]; since JD2443500 - see Table. BH Peg |P var. Max = 2426596.535 + 0.64101381d*E BH Peg |(JD2426500 - 28200) [01038]; since JD2434400 - see Table. BH Peg |Blazhko effect. A var. BH Peg |Max (O - C) = 2442929.03 + 39.8d*N [09588]. (k - b)2 = 0.09; BH Peg |Delta(S) = 5. BI Peg |Waves with a cycle of 60 - 80d are superimposed. BK Peg |Min II 10.47. BO Peg |Min II 11.6. P var. Min I = 2427655.460 + 0.5804342d*E BO Peg |(JD2426500 - 35100) [02263]; since JD2444000 - see Table. BP Peg |P1 = 0.084510d; P1:P0 = 0.77. Beat BP Peg |period Pb = 0.3698d [06604]. BU Peg |Observations are represented by the elements in the BU Peg |intervals JD2432000 - 34000, JD2438200 - 41400. BX Peg |Depth of Min II 0.62m; dI = 0.05P; dII = 0.00P. BX Peg |P var. Min I = 2431323.278 + 0.2804238d*E BX Peg |(JD2424700 - 39000) [00279]; since JD2439000 - see Table. BY Peg |P var. Min I = 2424745.75 + 0.34193403d*E BY Peg |(JD2424700 - 35400); since JD2435000 - see Table. CC Peg |Min II 12.9. CG Peg |Delta(S) = 2. P var? CU Peg |d = 0.010P. P var. Min = 2433895.463 + 3.8801345d*E CU Peg |(JD2425500 - 34000) [00001]; Min = 2434221.392 + CU Peg |3.880196d*E (JD2434000 - 36500) [07929]; CU Peg |since JD2436500 - see Table. CZ Peg |Min II 13.9. DF Peg |Min II 9.2. DG Peg |P var. Max = 2425857 + 148.15d*E (JD2425500 - DG Peg |33500); since JD2433500 - see Table. DH Peg |P var. Max = 2414981.537 + 0.25550478d*E DH Peg |(JD2414000 - 24000) [01158]; DH Peg |Max = 2427695.390 + 0.2555107d*E (JD2424000 - 33500) DH Peg |[09590]; since JD2433500 - see Table. [Fe/H] = -0.9. DI Peg |Min II 9.59. P var. Min I = 2425644.315 + 0.7118144d*E DI Peg |(JD2425500 - 30000) [02431]; Min I = 2437559.4096 + DI Peg |0.7118182d*E (JD2430000 - 40000) [09592]; Min I = DI Peg |2440159.6796 + 0.71181417d*E (JD2440000 - 44500); DI Peg |since JD2444500 - see Table. DK Peg |d = 0.04P. P var. Min = 2427745.388 + 1.631801d*E DK Peg |(JD2427700 - 33700); since JD2433700 - see Table. DM Peg |d = 0.03P; Min II 11.0. DN Peg |Mean brightness varies with cycles 800 - 1400d and DN Peg |A = 0.2m - 0.4m. DO Peg |P var. Min = 2434272.350 + 2.61394d*E (JD2428000 - 34700) DO Peg |[00485]; since JD2434700 - see Table. DV Peg |Min II 12.1. DY Peg |P var. Max = 2432751.9624 + 0.072926372d*E DY Peg |(JD2429000 - 38000); since JD2438000 - see Table. DY Peg |The basic pulsation is superimposed by the secondary one DY Peg |with P1 = 0.05570d [09594]. A var, M - m var (Pi = 0.2358d): DY Peg |0.55m < A < 0.67m, 0.24P < M - m < 0.42P. Delta(S) = 6. DZ Peg |P var. Max = 2429127.211 + 0.6073407d*E DZ Peg |(JD2419000 - 28800); Max = 2429127.189 + 0.6073761d*E DZ Peg |(JD2429100 - 33500); since JD2433500 - see Table. EE Peg |Min II 7.06. The third body (Porb = 1464d, T0 = 2443120). EF Peg |VB B (A 14.0m; B 5", 305deg). EH Peg |d = 0.08P. EQ PegA|VB A (B = EQb Peg; A = 6.87", Porb = 359 yr, E = 0.20. EQ PegA|[09597]); mu = 0.560", P = 91.7deg. A (B) >= 1.4m. EQ PegB|VB B (A = EQa Peg). a = 6.87'' P orb = 1464d, EQ PegB|T0 = 2443120. A(U) >= 1.9m. ET Peg |Delta(S) = 4. EU Peg |Min II 12.3. EZ Peg |On 1943 November 16 the spectrum of the star was B [02875]; EZ Peg |probably at that time the star had a flare. FL Peg |Min II 14.0. FU Peg |Blazhko effect (Pi = 150d); A var; FU Peg |15.2m <= Max <= 15.8m; 0.15P <= M - m <= 0.50P. GH Peg |Depth of Min II 0.13m. GR Peg |P var. Max = 2436492 + 69.93d*E (JD2436420 - 38740); GR Peg |since JD2440470 - see Table. GT Peg |mu = 0.51", P = 96deg. Epoch of the light minimum is given. GT Peg |During the flares A(U) < 3.6m. GV Peg |Delta(S) = 5:. GW Peg |Min II 15.1. GX Peg |SB1 (Porb = 2.340939d [06103]). GZ Peg |VB A (B 10.6m, A3V, 32.7", 198deg). HN Peg |[Fe/H] = -0.09. Epoch of light minimum is given. HN Peg |The variability of emission in H and K call lines with HN Peg |P = 4.63d was detected [09600]. HP Peg |Vr = -381 km/s. HR Peg |S4+/1+ . HZ Peg |Min II 17.6. II Peg |mu = 0.575", p = 86.5deg. SB1 II Peg |(T0 = 2443030.396 + 6.724464d*E); T0 is the epoch of the II Peg |inferior conjunction of K-star. The epoch of the II Peg |distortion wave maximum is given in the Table. Mean II Peg |brightness of the system varies. IK Peg |SB1 (Porb = 21.724d). Multiperiodicity [09609]. IM Peg |SB1 (Porb = 24.649d). QQ Peg |Variability needs confirmation. V0341 Peg |SB, Porb = 2.1779d. V0342 Peg |Suspected SB. bet Peg |VB A (B 11.2m, 109", 211deg). eps Peg |VB A (B 12.66m, 81", 325deg; C 8.65m, 140", 321deg). eps Peg |Usually varies in the range 2.29m - 2.44m V. On 1972 eps Peg |september 26/27 in the interval 23h58m - 00h02m UT it was eps Peg |bright (0.7m V), then at 00h09m UT decreased to 2.4m V eps Peg |[06875]. On 1847 November 5 the star was 3.5m, then the eps Peg |brightness increased but on November 6 it was still eps Peg |fainter than normal [09606]. tau Peg |P2 = 0.04895d; PB = 0.4943d. S Per |In the region of the open cluster h, khi Per. S Per |OH, H2O, SiO maser. S Per |In 1920 - 1969 there were secondary S Per |waves with cycles of 300d - 700d and Delta(m) ~1m [08630]; S Per |in 1935 - 1961 P1 = 807d, P2 = 930d [09694]. T Per |Other periodicities were noted. In the region T Per |of open cluster h, khi Per. U Per |P var. Max = 2411683 + 316.10d*E (before JD2422500); U Per |Max = 2422748 + 326.53d*E (JD2422500 - 34000); U Per |since JD2434000 - see Table. V Per |VB A (B 14m, 28", 278deg). W Per |P2 = 2667d +- 460d is superimposed. X Per |3U 0352 + 30. LX/Lopt = 10**(-2). ADS 2859 A (B = X Per |V397 Per, M3III, 22.5", 12deg). SB. X Per |IR excess. X-ray pulsar (P = 13.93m). X Per |Further periodicities were noticed in X-ray, optical, X Per |spectroscopic observations: 22.4h, 308.33d, 580.7d. Y Per |P var. Max = 2414990 + 254.74d*E (JD2415000 - 18000); Y Per |Max = 2418049 + 246.25d*E (JD2418000 - 22000); Y Per |Max = 2422242 + 253.62d*E (JD2422000 - 41000); Y Per |since JD2441000 - see Table. Z Per |d = 0.028P; Min II 9.8. Z Per |P var. Min = 2418173.663 + 3.056422d*E (JD2415000 - Z Per |19000) [01961]; Min = 2425481.416 + 3.05636d*E Z Per |(JD2419000 - 31000) [00978]; since JD2431000 - see Table. RR Per |P var. Max = 2424280 + 392.01d*E (JD2416000 - 28500); RR Per |since JD2428500 - see Table. RS Per |In the region of the open cluster h, khi Per. RS Per |According to [01053], P = 152d. RT Per |Min II 10.67. P var. Min = 2411963.2995 + 0.84941322d*E RT Per |(JD2411317 - 19400); Min = 2419702.3124 + 0.84940248d*E RT Per |(JD2419400 - 29300); Min = 2429751.6066 + 0.84941274d*E RT Per |(JD2429300 - 33000); since JD2433000 - see Table. RV Per |Min II 10.4. P var. Min = 2417972.345 + 1.973489d*E RV Per |(JD2417000 - 25500); since JD2432500 - see Table. RW Per |The light curve shape var, RW Per |d = 0.03P - 0.000P. Min II 9.78. P var. Before RW Per |JD2425720 Min = 2425720.0185 + 13.198910d*E; RW Per |Min = 2429217.5946 + 13.198399d*E (JD2425720 - 36700); RW Per |since JD2436700 - see Table. RY Per |d = 0.014P; Min II 8.65. RZ Per |S 3/7 e. P var. Before JD2430500 Max = 2415034 + 353.19d*E; RZ Per |since JD2430500 - see Table. ST Per |VB A (B 12.1m, 11.6", 6deg, 1928). d = 0.014P, Min II 9.62. ST Per |P var. Min = 2419030.5038 + 2.6483615d*E ST Per |(JD2418500 - 27000) [09740]; Min = 2429528.5897 + ST Per |2.6483488d*E (JD2427000 - 34600) [02389]; Min = ST Per |2439091.716 + 2.648353d*E (JD2439000 - 42400); ST Per |since JD2442400 - see Table. SU Per |In the region of the open cluster h, khi Per. SV Per |[A/H] = 0.6. SB2, hot companion. SV Per |P var? Before JD2435000 Max = 2419055.145 + SV Per |11.12875d*E [02431]; since JD2435000 - see Table. SX Per |[A/H] = 0. The chart in [08300] SY Per |In the region of the open cluster NGC 1528. TU Per |Delta(m), P var. Before JD2427200 Max = 2418572.288 + TU Per |0.6070775d*E; Max = 2427119.334 + 0.6070643d*E TU Per |(JD2427200 - 36000); since JD2436000 - see Table. TV Per |P2 = 1080d is superimposed. TX Per |[Fe/H] = -0.88. OH maser. TZ Per |VB A (B14m, 13", 290deg). Mu alpha = +0.012", TZ Per |mu delta = -0.050". In the region of the open TZ Per |cluster h, khi Per. UX Per |[A/H] = -0.3. UY Per |[A/H] = -0.3. In the region of the open clusters King 4, UY Per |Czernik 8. UZ Per |P2 = 91d is superimposed. VV Per |Twice shorter P is possible [00960]. VX Per |In the region of the open cluster h, khi Per. VX Per |[A/H] = -0.2. P var. Since JD2431000 - see Table. VY Per |In the region of the open cluster h, khi Per. VY Per |[A/H] = -0.3. VZ Per |VB A (B 16.9m pg, 17", 180deg). In the region of the open VZ Per |cluster Tr 2. WY Per |P var. Min = 2425234.460 + 3.327126d*E (JD2421500 - 26000) WY Per |[01072]; since JD2441500 - see Table. XX Per |VB A (B 9.7m vis, 21", 176deg, 1909). XX Per |Mean brightness var, P = 4100d. XY Per |ADS 2788 AB (delta(mV) = 0.6m - 2.5m, 1.4", 75deg, XY Per |SpA = A2II, SpB = B6e). IR excess. XZ Per |Min II 11.6. P var? Min = 2425150.439 + 1.1516282d*E XZ Per |(JD2425000 - 29000) [00522]; Min = 2437932.411 + XZ Per |1.1516347d*E + 0.005d*sin(0.09091deg*E) (JD2432000 - XZ Per |38000) [00001]; since JD2438000 - see Table. YZ Per |In the region of the open cluster h, khi Per. ZZ Per |The coordinates are possibly erroneous. AB Per |d = 0.045P; Min II 10.5. VB (Delta(m) = 0.0m vis, 0.20", AB Per |86.4deg, 1978). AD Per |Mean brightness var, P = 2950d. AD Per |In the region of the open cluster h, khi Per. AE Per |P2 = 2150d is superimposed. AG Per |ADS 2990 A (B Delta(m) = 2.0m, 0.9", 225deg, 1975; C 12.6m, AG Per |36", 118deg, 1948). The combined brightness AB is given. AG Per |Min II 7.00, DII = 0.10P, dII = 0. Apsidal motion: AG Per |Min II - Min I = 1.01435d + 0.0884d*sin(0.0278deg*E + AG Per |49.1deg). AR Per |P var, nonlinear term: +1.18d*10**(-11)*E**2. AR Per |[Fe/H] = -0.17. AS Per |Delta(m) var, d (Delta(B))/dt = -0.01m/yr. AV Per |P = 250 - 300d. AW Per |SB2, companion B6V, Delta(m) (companion - AW) = 2.8m vis. AX Per |Epoch of Min is given. The variability with Delta(m) up to AX Per |0.7m pg is caused probably by the orbital motion. Outburst AX Per |activity is superimposed. AY Per |d = 0.009P. BE Per |In the region of the open cluster CR 39. BI Per |In the region of the open cluster Berk 9. BL Per |P = 125 - 130d. BM Per |[Fe/H] = -0.04. BP Per |Min II = Min I. In the region of the open cluster BP Per |Cr 39. BU Per |Max brightness var, P = 8.1yr [01085]. In the region of BU Per |the open cluster h, khi Per. CC Per |Min II 14.1. CI Per |P var (3.35d - 3.40d), possibly with a period of 4000d. CI Per |The light curve shape var. CK Per |d = 0.05P:. CM Per |d = 0.052P. In the region of the open cluster Stock 2. CO Per |In the region of the open cluster Stock 2. CR Per |Elements need confirmation. In the region of the open CR Per |cluster Stock 2. CS Per |In the region of the open cluster Stock 2. CZ Per |In the region of the open cluster h, khi Per. DE Per |d = 0.01P? DF Per |In the region of the open cluster h, khi Per. DG Per |d = 0.021P. DK Per |The depth of Min II 0.05m. In the region of the open DK Per |cluster h, khi Per. DM Per |Min II 8.02, DII = 0.17P. DM Per |Depths of Minima, the shape of Min II var. DM Per |In the region of the open cluster h, khi Per. DO Per |In the region of the open cluster h, khi Per. DP Per |In the region of the open cluster h, khi Per. DR Per |In the region of the open cluster h, khi Per. DS Per |In the region of the open cluster h, khi Per. DT Per |In the region of the open cluster h, khi Per. DU Per |In the region of the open cluster h, khi Per. DV Per |Min II 14.5. DY Per |In the region of the open cluster Tr 2. DZ Per |Min II 14.7. In the region of the open cluster Tr 2. EL Per |Before JD2428900 Max = 2427980 + 167d*E; EL Per |during JD2428900 - 31000 - see Table. EO Per |IR excess? ER Per |Mean brightness var, P ~900d. EU Per |Min brightness var, P ~900d. EW Per |Superimposed waves 70d - 180d. EW Per |In the region of the open cluster Stock 4. EX Per |Min II 12.5. FM Per |VB A (B 12.1m, 3", 285deg). P var? Max = 2429982.268 + FM Per |0.489199d*E (JD2428000 - 30600); FM Per |During JD2433700 - 36000 - see Table. FR Per |In the region of the open cluster NGC 1528. FV Per |Cycles 300 - 350d, 1800d:. FX Per |d = 0.04P. In the region of the open cluster NGC 1582. FY Per |Possible periods 0.0702d, 0.4407d. FY Per |Photometric spectral type B1V. FZ Per |In the region of the open cluster h, khi Per. GH Per |P = 220d is possible. GK Per |SB2 (sdBE + K2IVp). GK Per |The following types of activity are being observed after GK Per |the return to the normal brightness: rapid irregular GK Per |variations (Delta(m) ~0.1m in several minutes); irregular GK Per |fluctuations from night to night (Delta(m) up to 0.3m); GK Per |slow irregular variations (Delta(m) = 1.5m in several GK Per |dozen days); bursts with light increase in 10d - 30d and GK Per |decrease in 10d - 40d, Delta(m) up to 3.5m, the mean GK Per |interval between bursts being delta(t) = 820d [09686,09788]. GK Per |According to [10198], the radial velocities are GK Per |represented with the elements Max (Vr > 0) = 2444912.966 + GK Per |1.996803d*E (Kabs = 124 km/s, Kem = 34 km/s). According GK Per |to [10199], the 2d variation is modulated with a period GK Per |of 0.131623d, Max (delta(Vr)) ~2443787.995 (Kabs = GK Per |15 km/s, Kem = 20 km/s). During a burst the sinusoidal GK Per |modulation of X-ray flux was recorded, GK Per |Tmax = 24455555.67456 + 0.004066443d*E [09786]. GK Per |ExpAnding envelope (0.454"/yr, 1948 - 1964; GK Per |0.432"/yr, 1964 - 1981, [09787]). GP Per |[A/H] = -0.5. GQ Per |According to [00021], Sp K0. HQ Per |[A/H] = -0.3. HS Per |In the region of the open cluster Stock 4. HV Per |d ~0.03P. HW Per |Min II 13.3. Min II - Min I = 0.45P:. HY Per |Three of the four min in [01079] are not satisfied with the HY Per |elements. HZ Per |[A/H] = -0.8. B_V: +1.93, +2.34. II Per |Min II 13.6. In the region of the open cluster NGC 1582. IK Per |Min II 11.6. IM Per |Min II 12.7. The elements need confirmation. In the region IM Per |of the open cluster Cr 39. IO Per |H2O maser. IP Per |IR excess. IQ Per |dI = 0.02P. Min II 7.88, DII = 0.12P, dII = 0.03P, IQ Per |Min II - Min I = 0.53P. P var? VB A (B = BD + 47deg 921, IQ Per |9.30m, A0V np:, 39.3", 175deg); SB1. IT Per |dI = 0.06P. Min II 10.0, DII = 0.24P:, dII = 0.16P:. IT Per |VB (Delta(m) = 1.7m, 12", 37deg). IT Per |The range of the combined brightness is given. IW Per |SB1. Min II 5.83. IX Per |The depth of Min II 0.02m. IX Per |VB A (B 10.6m, 5", 208deg). IZ Per |Min II 8.3. KK Per |In the region of the open cluster h, khi Per. KP Per |Beat phenomenon: P1 - see Table, KP Per |A1 = 0.0323m B; P2 = 0.1980855d, A2 = 0.0235M B; P3 = KP Per |0.2270986d, A3 = 0.0072M B. KR Per |Min II 11.1. KS Per |SB (Porb = 360.47d). KS Per |The main component is a helium star. Besides the KS Per |semiregular variability (see Table), variations were noted KS Per |with P = 50 - 100 Min and Delta(m) of several hundredths KS Per |of a magnitude. IR excess. Variable polarization (P - 1%). KT Per |Quasi-periodic oscillations during outbursts: P = KT Per |22.9s - 29.5s [05959], 82s, 90s, 147s [09791], Delta(m) KT Per |up to ~0.01m. KV Per |[Fe/H] = -0.96. P var. Max = 2428950.400 + 0.24942d*E KV Per |(JD2428950 - 29200); since JD2429500 - see Table. KW Per |Min II 10.8. P var. Min = 2426295.450 + 0.931255d*E KW Per |(JD2423400 - 39500) [04009]; since JD2440000 - see Table. KY Per |In the region of the open cluster h, khi Per. KZ Per |In the region of the open cluster h, khi Per. LL Per |In the region of the open cluster h, khi Per. LM Per |In the region of the open cluster h, khi Per. LN Per |In the region of the open cluster h, khi Per. LO Per |In the region of the open cluster h, khi Per. LP Per |In the region of the open cluster h, khi Per. LQ Per |In the region of the open cluster h, khi Per. LR Per |Very red. In the region of the open cluster h, khi Per. LX Per |mu alpha = +0.0065s, mu delta = -0.063". Min II 8.38m. LX Per |DII = 0.05P. Migrating distortion wave: LX Per |P = 475d [09792], Delta(m) up to 0.04m. MS Per |Min II 12.1. MX Per |IR excess. NP Per |Min II 13.0. NR Per |P var. Max = 2416780 + 323.0d*E (JD2415750 - 24550); NR Per |Max = 2435060 + 340.2d*E (JD243350 - 35400); NR Per |since JD2436700 - see Table. NU Per |A close pair, var is the southern star. OV Per |D ~2h. PP Per |In the region of the open cluster h, khi Per. PR Per |In the region of the open cluster h, khi Per. QR Per |Red. QU Per |d = 0.03P. QW Per |Min II 14.7:. QX Per |Min II 16.1. V0345 Per |In the nebula NGC 1579. V0346 Per |In the nebula NGC 1579. V0347 Per |In the nebula NGC 1579. V0351 Per |In the region of the open cluster h, khi Per. V0352 Per |In the region of the open cluster h, khi Per. V0354 Per |In the region of the open cluster h, khi Per. V0355 Per |In the region of the open cluster h, khi Per. V0356 Per |In the region of the open cluster h, khi Per. V0357 Per |In the region of the open cluster h, khi Per. P = 0.21955d V0357 Per |is possible. V0358 Per |In the region of the open cluster h, khi Per. V0359 Per |In the region of the open cluster h, khi Per. V0360 Per |In the region of the open cluster h, khi Per. V0360 Per |Other possible periods: 0.40036d, 0.40154d. V0361 Per |In the region of the open cluster h, khi Per. V0363 Per |Red. V0364 Per |Min II 15.6, Max II 14.8. V0365 Per |Min II 14.3:. V0376 Per |P2 = 0.09165d, A2 = 0.016m; P1 - see Table, V0376 Per |A1 = 0.037m. A var. V0380 Per |SB (Porb = 26d?). The epoch of Min light is given. V0382 Per |In the region of the open cluster h, khi Per. V0392 Per |The southern component of a very close pair. V0394 Per |H2O maser. V0395 Per |VB A (B 3.5", 90deg). V0396 Per |In the region of the open cluster alpha Per. V0396 Per |Observations are also satisfied by P ~1.678d. According V0396 Per |to [07586], P = 2.4928d or 1.6857d. V0397 Per |ADS 2859 B (A = X Per; B 22.5", 12deg). V0398 Per |IN type is also possible. V0403 Per |In the region of the open cluster h, khi Per. V0409 Per |Epoch of Min is given. V0423 Per |ADS 2433 A (B 11.9m, 30.8", 99.2deg); SB. V0423 Per |Porb is given. V0424 Per |In the region of the open cluster h, khi Per. IR excess. V0425 Per |VB A(B 12.8m, 3.6", C 14.3m, 6.8"). In the region of V0425 Per |the open cluster h, khi Per. V0428 Per |According to [08639], type IS? V0432 Per |Min II 11.6. V0434 Per |Min II 14.9. V0436 Per |Min II 5.74; Min II - Min I = 0.413P; D II = 0.03P. V0437 Per |In the region of the open cluster NGC 744. V0438 Per |In the region of the open cluster h, khi Per. VB (8.7m, V0438 Per |10.9m, 1".2, 26deg). V0438 Per |Min II 8.34. The range of combined brightness V0438 Per |variation is given. The bright component is V0438 Per |considered to be variable. This suggestion V0438 Per |needs verification. V0439 Per |In the region of the open cluster h, khi Per. V0440 Per |In the region of the open cluster h, khi Per. ADS 1820 V0440 Per |A (B 14.5m, 8".3, 122deg). V0449 Per |Min II 13.3. V0451 Per |Min II 15.8. V0459 Per |In the alpha Per cluster. V0461 Per |In the alpha Per cluster. V0462 Per |Min II 14.0. V0465 Per |P2 = 0.030d is superimposed. V0466 Per |Superposition of P1 = 5300d +- 250d, P2 = 475d +- 35d V0466 Per |(Delta(m) = 1.1m), P3 = 0.26d (Delta(m) = 0.5). V0468 Per |P1 = 925s, P2 = 1022s. mu = 0".29, p = 170deg. V0469 Per |Changes of line profiles with periods 0.150d, 0.188d, V0469 Per |0.304d, 0.476d, 0.608d, 1.88d [09814]. V0469 Per |In 1978/1979 non-radial pulsations were observed: V0469 Per |P1 = 1.74d. P2 = 2.04d [04173,04180]. V0470 Per |VB A (B 18.8m B, 1" - 2"). V0471 Per |The central star of the planetary nebula M1-2 = VV8. V0471 Per |According to [09815,09816], const. V0547 Per |High proper motion (LTT 10610) not confirmed by HIPPARCOS data. V0580 Per |The variability may be due to the fainter (B) component. V0582 Per |A single deep minimum at the bottom of the small-amplitude V0582 Per |(5.63 - 5.64) wave. V0592 Per |VB (0".2, 197 deg, 1989.7). bet Per |Multiple system (Eclipsing pair = Algol AB; Algol C 4.7m, bet Per |Am, a = 0".10, Porb = 1.862a); Algol AB = ADS 2362 A bet Per |(B 12.7m, 57".5, 156deg, 1920). P var. P = 2.8673442d bet Per |(1784 - 1835); P = 2.8673012d (1835 - 1854); bet Per |P = 2.8672775d bet Per |(1854 - 1901); P = 2.8672967d (1901 - 1913); bet Per |P = 2.8672506d bet Per |(1913 - 1915) [06156]; Min I = 2424477.806 + 2.86730236d*E bet Per |(JD2420500 - 25000); Min = 2425917.203 + 2.86732697d*E bet Per |(JD2425000 - 277000); Min I = 2433194.454 + 2.86731667d*E bet Per |(JD2427700 - 33600); Min I = 2433928.4944 + 2.86732442d*E bet Per |(JD2433600 - 37000); Min I = 2437598.6766 + 2.86733732d*E bet Per |(JD2437000 - 42200); since JD2442200 - see Table. bet Per |Porb (Algol C) = 1.862a may be traced in the deviations; bet Per |a period of 32a may also be real. Depth of Min I var. bet Per |Variable polarization, changes in hydrogen line profiles, bet Per |sometimes emissions in the spectrum. Radio source with bet Per |frequent burst of different amplitude, faint X-ray source. del Per |Variable emission lambda 1650 A [06905]. Vr var, del Per |A = 16 km/s. ksi Per |In the far IR range (lambda = 10 mkm) Delta(m) > 1m. In ksi Per |the far IR range (lambda = 10 mkm ) Delta(m) > 1m; the ksi Per |variability is related to mass loss. omi Per |VB A (B 8.4m, 0.96'', 29.7deg,1972). Possible omi Per |superposition of BCEP type oscilations. rho Per |A slower variation of the mean light is possible. rho Per |mu alpha = 0.0111s, mu delta = -0.102''. phi Per |SB2. (Porb = 126.696d). v*sin(i) = 450km/s. A var (P ~Porb). b Per |SB2. Depths of minima differ by 0.03m. Third body? , b Per |P = 701d. Radio source. In the region of the open cluster b Per |NGC 1545. R Phe |P var. Max = 2405121 + 271.0d*E(JD2405000 - 11500); R Phe |Max = 2414570 + 266.26d*E(JD2414500 - 25500); R Phe |since JD2425500 - see Table. T Phe |P var. Max = 2411252 + 281.00d*E(JD2410000 - 30000); T Phe |since JD2430000 - see Table. W Phe |P var. Max = 2414960 + 328.65d*E(JD2414500 - 19500); W Phe |Max = 2424530 + 332.87d*E(JD2424500 - 30200); W Phe |since JD2436000 - see Table. RS Phe |P var? RT Phe |P = 208d? RV Phe |P var?; (k-b)2 = 0.06; Delta(S) = 8: SX Phe |mu = 0.894", ro = 163.1deg. P var. Max = 2433923.9618 + SX Phe |0.054964519d*E1 - 0.00337d*sin(2pi*(0.28503379*E1 + 0.074)) SX Phe |(JD2433900 - 36900); since JD2436900 - see Table. SX Phe |There is a periodic term in the elements given in the SX Phe |Table: -0.00325*sin(2pi*(0.28503575*E2 - 0.107)). According SX Phe |to [09614] for epoch 1950.0 P0 = 0.054964509, SX Phe |P1 = 0.042772831, Pb = 0.1928355; dP0/dt = -87*10**(-13), SX Phe |dP1/dt = -174*10**(-13), dPb/dt = 2.46*10**(-10). SX Phe |P1/P0 = 0.778; 0.8m <= A <= 0.3m; SX Phe |0.2p <= M-m <= 0.4p. [Fe/H] = -0.6. WW Phe |Min II 12.7. YZ Phe |Min II 13.0. AD Phe |Min II 10.80. P var. Min I = 2436847.375 + 0.3799277*E AD Phe |(JD2428650 - 36850); since JD2436850 - see Table. AE Phe |Min II 8.19; 0.033p <= dI <= 0.05p; dII = 0.00. The AE Phe |shape of the light curve varies with periods 55.9d and AE Phe |95.3d [09615]. P var. Min I = 2440857.8140 + 0.36237459*E AE Phe |(JD2438250 - 40870) [07388]; Min I = 2441969.57074 + AE Phe |0.36237186d*E (JD2440870 - 42000) [09616]; Min I = AE Phe |2442654.8201 + 0.3623741d*E (JD2441950 - 42660) [09533]; AE Phe |since JD2443700 - see Table. AG Phe |Min II 8.95. P var. Min I = 2440415.231 + 0.7553429d*E AG Phe |(JD243800 - 40850); since JD2443750 - see Table. AI Phe |Min II 8.89; dI = 0.0035; Min II - Min I = 0.46p. AU Phe |Min II 13.0. According to [09517] the P value given in AU Phe |the Table is wrong. AX Phe |mu = 0.234", p = 70deg. Multiperiodical: P i = 606.8s, AX Phe |682.7s, 744.7s, 840.2s (Ai ~0.01m). CG Phe |Type RRC: is also possible. gam Phe |SB1 (P orb = 193.85d). zet Phe |VB A (B 7.0m, A7:, 0.46", 51.4deg, 1965.9; C 8.0m, zet Phe |F7V, 6.4"). Total light range of A and B components is zet Phe |given in the Table. Min II 4.22, MinII - MinI = 0.507p; zet Phe |dII = 0.02p. iot Phe |VB A (B 12.7m, 7.7", 270deg). ksi Phe |VB A (B 12.1m, 13.2", 253deg). Epoch of MinI(v) is given ksi Phe |in the Table. A(v) = 0.13m. rho Phe |Frequency analysis results see also in [09619,09620,9621]. psi Phe |SB. R Pic |P var. Max = 2413413 + 165.8d*E (JD2413000 - 23600); R Pic |since JD2423600 - see Table. Light curve (1923 - 1953) R Pic |[01054]. S Pic |P var. Max = 2413595 + 424.7d*E (JD2405500 - 23000); S Pic |since JD2423000 - see Table. OH emission. U Pic |P var. Max = 2428103.565 + 0.44036450*E (JD2414000 - U Pic |29000) [00353]; since JD2438400 - see Table. (k - b)2 = U Pic |0.17; Delta(S) = 3. X Pic |Min II 10.8 RR Pic |Since 1965 periodic light variations were detected RR Pic |with A(B) = 0.33m and elements Max = 2438815.380 + RR Pic |0.14502545d*E. These variations are superimposed by RR Pic |others with A(B) = 0.036m and period ~15.6 min or RR Pic |15.4 min [09612]. There are also rapid oscillations RR Pic |with periods in the range 20 - 40s [09613]. RT Pic |Not seen only on one plate; defect? RV Pic |Min II 9.79. SU Pic |Min II 10.4. VW Pic |Variability may be due to component B. VZ Pic |Kapteyn's star. del Pic |Min II 4.83. R Psc |P var. Max = 2418070 + 344.14d*E (JD2397070 - 27700); R Psc |Max = 2432866 + 347.1d*E(JD2427300 - 33000) - see Table. S Psc |P var. Max = 2406665 + 405.6d*E (JD2398944 - 2407100); S Psc |Max = 2415930 + 402.6d*E (JD2407100 - 16500); Max = S Psc |2421295 + 413.7d*E (JD2416500 - 21500) - see Table. U Psc |P var. Max = 2417230 + 172.71d*E (JD2407720 - 18000); U Psc |Max = 2423840 + 174.3d*E (JD2418000 - 24000) [00001]; U Psc |Max = 2424527 + 170.3d*E (JD2423000 - 26100) [00960]; U Psc |Max = 2432514 + 174.05d*E (JD2425000 - 33000) [00001]; U Psc |since JD2433000 - see Table. V Psc |mu alpha = 0.0112s, mu delta = -0.215". W Psc |P var. Max = 2412690 + 189.08d*E (JD2412692 - 27100) W Psc |[01193]; W Psc |since JD2435000 - see Table. X Psc |P var. Max = 2433474 + 357.3*E (JD24295000 - 38000); since X Psc |JD2438000 - see Table. Y Psc |P var. Min = 2410002.844 + 3.76582d*E (JD2410000 - 19700) Y Psc |[09707]; Min = 2425495.522 + 3.765903d*E Y Psc |(JD2423200 - 6300) [01072]; Min = 2430613.384 + Y Psc |3.7658895d*E Y Psc |(JD2427300 - 30620); Min = 2432865.357 + 3.7658405d*E Y Psc |(JD2430620 - 32900); Min = 2435693.452 + 3.7657765d*E Y Psc |(JD2432860 - 36600) [00001]; Min = 2441225.473 + Y Psc |3.765859d*E Y Psc |(JD2439000 - 42500) [06956]; Min = 2443142.29056 + Y Psc |3.7658491d*E (JD2442500 - 44000) [08593]; since JD2444000 - Y Psc |see Table. RS Psc |In the region of the galaxy NGC 251. RT Psc |Mean brightness varies with P2 = 533d. According to [08643] RT Psc |30d <= P1 <= 70d. RU Psc |[Fe/H] = -1.65. P var. [00752,09714] Max = 2415407.609 + RU Psc |0.3903008d*E (JD2414400 - 15700); Max = 2416022.660 + RU Psc |0.3902139d*E (JD2415700 - 16600); Max = 2417244.537 + RU Psc |0.3902878d*E (JD2416600 - 19200); Max = 2419936.853 + RU Psc |0.3903520d*E (JD2419200 - 22000); Max = 2425894.778 + RU Psc |0.3903016d*E (JD2422000 - 26200); Max = 2426214.829 + RU Psc |0.3903546d*E (JD2426200 - 27300); Max = 2427397.519: + RU Psc |0.3902216d*E (JD2427300 - 28000); Max = 2428165.524 + RU Psc |0.3903535d*E (JD2428000 - 29300); Max = 2429488.868: + RU Psc |0.3904577d*E (JD2429300 - 600) [00752]. Max = 2430053.353 + RU Psc |0.390202d*E (JD2430000 - 650); Max = 2430935.366 + RU Psc |0.390354d*E (JD2430600 - 940); Max = 2431331.307 + RU Psc |0.390457d*E (JD2430940 - 31350); Max = 2432119.417 + RU Psc |0.390346d*E (JD2431350 - 32120); Max = 2433162.250 + RU Psc |0.390283d*E (JD2432100 - 33200); Max = 2433905.311 + RU Psc |0.390261d*E (JD2433200 - 33910); Max = 2433905.311 + RU Psc |0.390321d*E (JD2433900 - 35430); Max = 2435429.502 + RU Psc |0.390412d*E (JD2435420 - 35800); Max = 2435781.265 + RU Psc |0.39027d*E (JD2435780 - 36130); Max = 2436501.361 + RU Psc |0.39032d*E (JD2436130 - 36510); Max = 2436534.190 + RU Psc |0.39043d*E (JD2436500 - 36850); Max = 2436845.351 + RU Psc |0.39025d*E (JD2436840 - 37200); Max = 2437181.358 + RU Psc |0.39031d*E (JD2437180 - 37610); Max = 2437994.329 + RU Psc |0.39026d*E (JD2437610 - 38000); [00001]. RU Psc |Max = 2438303.950 + 0.39040d*E (JD2438000 - 38400) [03879]. RU Psc |Max = 2438375.409 + 0.39027d*E (JD2438370 - 38650) [00001]. RU Psc |Max = 2439435.2421 + 0.390385d*E (JD2438650 - 39500) RU Psc |[09713]. Max = 2439435.242 + 0.390313d*E (JD2439430 - 39800); RU Psc |Max = 2439771.3049 + 0.39046d*E (JD2439770 - 40140) [00001]. RU Psc |Since JD2440140 - see Table. According to [03569] A var RU Psc |with P = 28.8d. RV Psc |Min II 12.0. RY Psc |(k-b)2 = 0.03, Delta(S) = 7. P var. Max = 2419677.268 + RY Psc |0.52971027d*E (JD2414000 - 22000); Max = 2425148.192 + RY Psc |0.52972643d*E (JD2422000 - 25500) [01337]; Max = RY Psc |2425508.390 + 0.5297291d*E (JD2425500 - 40000); RY Psc |Max = 2441538.476 + 0.52972911d*E (JD2441000 - 41650) RY Psc |[07984]; since JD2442660 - see Table. RZ Psc |Algol-like. SS Psc |(k-b)2 = 0.19; Delta(S) = 2. Blazhko effect: SS Psc |-0.04d <= O-C <= +0.04d; Min(O-C) = 2437520 + 136d*E SS Psc |[09731]. SU Psc |Min II 11.3. SW Psc |P var. Max = 2425177.298 + 0.5212844d*E (JD2419670 - SW Psc |25200) [04191]; Max = 2425177.256 + 0.5212642d*E SW Psc |(JD2425170 - 38000) [03506]. Since JD2438600 - see Table. SW Psc |There is a periodic term in the elements given in the SW Psc |Table: + 0.0132d*sin(5.440deg*(E + 2)). Blazhko effect SW Psc |(Pi = 34.5d). SX Psc |P var. Min = 2427811.357 + 0.825882d*E (JD2425580 - 36000) SX Psc |[01218]; Min = 2437202.453 + 0.825877d*E SX Psc |(JD2436000 - 39900) SX Psc |[00001]; since JD2439800 - see Table. SZ Psc |Min II 7.38. P var. SZ Psc |There is a square term in the elements given in the Table: SZ Psc |-0.113d*10**(-6)*E**2. TY Psc |Porb = 0.080d [09735]. TY Psc |The cycle of supermaxima is 370d [09675]. UU Psc |VB A (B 7.60m, F4V, 11.5", 148deg, 1966.9). Min II 6.04; UU Psc |Min II - Min I = 0.55P. UU Psc |Elliptical orbit and rotation of the line of apsides are UU Psc |possible. UV Psc |Min II 9.54. P var. Min I = 2424134.574 + 0.8610475d*E UV Psc |(JD2414600 - 24150) [00001]; Min I = 2428038.555 + UV Psc |0.861046d*E (JD2424150 - 36700) [02924]; UV Psc |since JD2436700 - see Table. The shape of the light UV Psc |curve varies. UW Psc |Min II 11.0:. UZ Psc |SB1 (Porb > 1 yr [05751]). VZ Psc |Mu = 0.43", P = 65deg. Min II 10.43. WW Psc |VB A (B 13.1m, 31"). WX Psc |OH, H2O, SiO maser. ZZ Psc |P1 = 612s, P2 = 816s [07476]. ZZ Psc |Nonradial modes [08467]. AG Psc |P (Vr) = 0.055d. AH Psc |The star was seen in 1854 - 60; since 1862 it was not AH Psc |observed. AO Psc |Epoch of Max brightness is given. Light variations with AO Psc |Porb = 0.1496263d are superimposed by variations with AO Psc |P = 858.6861s and twice smaller amplitude (Max = AO Psc |2444815.00276 + 0.009938496d*E; M-m = 0.54P), and AO Psc |also by still smaller oscillations with P = 805.2059s AO Psc |(Max = 2444815.00294 + 0.009319513d*E). The last period AO Psc |is the X-ray impulse period which is equal to AO Psc |the period of rotation of the compact object (probably AO Psc |a white dwarf). R PsA |P var. Max = 2417385 + 293.00d*E (JD2405000 - 26000); R PsA |Max = 2432896 + 291.50d*E (JD2426000 - 38000); R PsA |since JD2438000 - see Table. S PsA |P var. Max = 2417853 + 271.0d*E (JD2411000 - 18000); S PsA |Max = 2426880 + 273.6d (JD2418000 - 27000); Max = S PsA |2434714 + 270.3d (JD2427000 - 35000); since S PsA |JD2434000 - see Table. X PsA |Min II 14.2. RW PsA |Min II 11.63. TX PsA |VB B (A 13.0m pg; B 37", 131deg); mu = 0.22", p = 117deg. pi PsA |SB (Porb = 178.3177d [05769]). R Pup |In the region of the open cluster NGC 2439. U Pup |P var. Max = 2415090 + 314.26d*E (JD2408000 - 22800); U Pup |since JD2422800 - see Table. V Pup |VB A (B 10.0m, 7", 0, 70deg; C 11.0m, 19.0", 48deg). V Pup |Min II 4.82. P var. IO - CI < 0.02d. W Pup |P var. Max = 2420990 + 120.68d*E (JD2412500 - 23600); W Pup |Max = 2424725 + 119.9d*E (JD2423600 - 26300); W Pup |Max = 2432200 + 120.68d*E (JD2426300 - 40800); W Pup |since JD2440800 - see Table. X Pup |P var. Max = 2414889.8 + 25.939d*E (JD2408800 - 16000); X Pup |Max = 2435188.76 + 25.9610d*E (JD2419000 - 35190) X Pup |[02392]; Max = 2436279.50 + 25.97d*E X Pup |(2435190 - 38000) [00001]; since JD2438000 - see Table. Z Pup |OH, H2O, SiO emission. Z Pup |P var. Max = 2424256 + 513.90d*E (JD2413900 - 24500); Z Pup |since JD2424500 - see Table. RS Pup |Surrounded by the reflecting nebulosity with a radius of RS Pup |1.4' [09634]. P var. Max = 2419186.3 + 41.337d*E RS Pup |(JD2414000 - 24000) [02049]; Max = 2427083.613 + 41.414d*E RS Pup |(JD2425800 - 28300) [02440]; Max = 2434823.23 + 41.38535d*E RS Pup |(JD2433750 - 34900) [09636]; since JD2435700 - see Table. RW Pup |P var. Max = 2430175 + 332.5d*E (JD2424500 - 30200) RW Pup |[00001]; since JD2435800 - see Table. RX Pup |Light curve (1890 - 1925) [01265]. RX Pup |Mira type component light variations are observed in the RX Pup |infrared region of spectrum: Max = 2444530 + 580d*E, RX Pup |3.99m - 6.00m J, M - m = 0.50P [09518]. ST Pup |[A/H] = -0.9. ST Pup |The light curve shape and the period vary strongly: ST Pup |0.10P < M - m < 0.30P; 17.4d < P < 19.19d. ST Pup |P = 19.188d (JD2415000 - 17000); 18.949d ST Pup |(JD2417000 - 18000), 18.8065d (JD2418000 - 19000), ST Pup |18.721d (JD2419000 - 20000), 18.714d (JD2420000 - 21000), ST Pup |18.717d (JD2421000 - 22000), 18.6175d (JD2422000 - 23000), ST Pup |18.678d (JD2423000 - 24000), 18.735d (JD2424000 - 25000), ST Pup |18.796d (JD2425000 - 26000), 18.817d (JD2426000 - 27000) ST Pup |[01266]. Max = 2427779.6 + 18.846d*E (JD2427000 - 28000) ST Pup |[01266]; Max = 2428893.9 + 18.885d*E (JD2428000 - 29000) ST Pup |[00016]; Max = 2429697.51 + 19.188d*E (JD2429000 - 30000) ST Pup |[01266]. P = 19.142d (JD2430000 - 31000), ST Pup |19.145d (JD2431000 - 32000) [01266]. ST Pup |Max = 2435395.430 + 18.559d*E (JD2435160 - 500) ST Pup |[06006]; Max = 2435617.45 + 18.8864d*E (JD2435500 - 5620) ST Pup |[02309]; Max = 243957.3 + 17.4d*E (JD2438700 - 39600) ST Pup |[06611]; since JD2444000 - see Table. SV Pup |P var. Max = 2419010 + 166.6d*E (JD2413660 - 18000); SV Pup |Max = 2423090 + 169.8d*E (JD2418000 - 23100); SV Pup |Max = 2426782 + 167.8d*E (JD2423100 - 27500); SV Pup |since JD2427500 - see Table. SW Pup |Min II 9.1; d = 0.029P. TT Pup |Min II 13.6. TY Pup |Min II 8.87. UZ Pup |Min II 10.0. VV Pup |mu = 0.100", P = 165.0deg. VV Pup |The epoch of light maximum is given. The mean VV Pup |brightness varies by 2 - 3m. Intervals of active light VV Pup |variation with amplitude up to 2m during maximal mean VV Pup |brightness are observed. During low activity intervals VV Pup |when amplitude is about 0.3m mean brightness is minimal; VV Pup |during this time the ellipsoidal light variations of the VV Pup |system are observed in the range 15.1m - 15.3m J with the VV Pup |elements Min = 2427889.6509 + 0.0697468256d*E [09644]. VV Pup |The white dwarf rotation period is equal to the orbital VV Pup |period. There are flickerings. Spectrum description VV Pup |[09472,09645]. VW Pup |P var. Max = 2425184.67 + 4.28405d*E (JD2422660 - 25600) VW Pup |[00973]; Max = 2435554.86 + 4.28519d*E (JD2425600 - 35600) VW Pup |[02309]; since JD2435500 - see Table. VX Pup |P1 = 2.1389d (A1 = 0.29m); A0 = 0.31m; P1/P0 = 0.71042. VY Pup |The depth of Min II 0.04m. VZ Pup |[A/H] = -0.3. P var. Max = 2434864.90 + 23.1640d*E VZ Pup |(JD2426700 - 35300) [02309]; since JD2435300 - see Table. WW Pup |P var. Max = 2424497.73 + 5.5159d*E (JD2423520 - WW Pup |26000) [00973]; since JD2426000 - see Table. WX Pup |P var. Max = 2435042.184 + 8.93825d*E (JD2422000 - WX Pup |35100) [02431]; since JD2435000 - see Table. WZ Pup |P var. Max = 2427861.33 + 5.02657d*E (JD2421100 - WZ Pup |29400) [02392]; since JD2429400 - see Table. XX Pup |P var. Max = 2426338.503 + 0.51719805d*E XX Pup |(JD2426300 - 39500) [03572]; since JD2441700 - see Table. XX Pup |(k - b)2 = 0.07. The spectral type according to CA II is XX Pup |given. XY Pup |Min II 9.4; d = 0.042P. XZ Pup |Min II 7.90. P var. Min I = 2440629.7969 + 2.192383d*E XZ Pup |(JD2425850 - 41700) [00099]; since JD2441700 - see Table. YY Pup |The depth of Min II 0.05m. AE Pup |In the region of the open cluster Cr 173. AF Pup |Min II 13.5. AG Pup |Min II 10.9. AH Pup |The depth of Min II 0.05m. AN Pup |Min II 10.7. AQ Pup |VB A (B 11.13m, < 15"; C 12.83m, < 15"). [A/H] = -0.1. AQ Pup |The range of the variation of combined light is given. AQ Pup |P var. Max = 2429734.59 + 29.931d*E (JD2427500 - 33000) AQ Pup |[03474]; Max = 2433296.2 + 30.018d*E (JD2433000 - 35850) AQ Pup |[02474]; Max = 2436625.9 + 29.8568d*E AQ Pup |(JD2435850 - 36700) [03601]; Max = 2441760.63 + 30.032d*E AQ Pup |(JD2436600 - 42700) [09671]; since JD2443400 - see Table. AR Pup |The mean brightness varies with P = 1200d. AS Pup |In the region of the open cluster NGC 2546. P var. AS Pup |Max = 2416110 + 331.4d*E (JD2415460 - 26000); since AS Pup |JD2426000 - see Table. AT Pup |In the region of the open cluster NGC 2546. AT Pup |P var. Max = 2426758.205 + 6.6648d*E (JD2426700 - 35600) AT Pup |[02202]; since JD2435600 - see Table. AU Pup |Min II 9.28. P var. Min I = 2428111.304 + 1.126418d*E AU Pup |(JD2414700 - 28200) [00007]; since JD2439000 - see Table. AV Pup |Min II 11.0. AW Pup |VB A (B 11.7m, 3.7", 258deg). Period probably must be AW Pup |doubled. AY Pup |Min II 12.5. AZ Pup |Min II 10.1. BB Pup |(k - b)2 = 0.24; Delta(S) = 3. BH Pup |In the region of the open cluster Cr 173. BI Pup |In the region of the open cluster Cr 173. BK Pup |In the region of the open cluster Cr 173. BL Pup |Min II 14.2. BN Pup |In the region of the open cluster NGC 2533. BP Pup |Min II 12.3. BQ Pup |The shape of the light curve possibly varies. BR Pup |Min II 12.9. BT Pup |Min II 14.5. In the region of the open cluster NGC 2482. BU Pup |Min II 13.9. In the region of the open cluster NGC 2447. BW Pup |The depth of Min II 0.15m. BX Pup |In the region of the open cluster NGC 2482. CE Pup |P var? [07934]. CH Pup |P var. Max = 2428465 + 491.0d*E (JD2428400 - 37300); CH Pup |since JD2437300 - see Table. CO Pup |P var? The epoch of light minimum is given. CP Pup |In 1981 the radius of the shell expanding with CP Pup |Vexp = 710 km/s was equal to 7" [09689,09559]. CX Pup |d = 0.05P. CY Pup |d = 0.01P:; Min II 13.0. CZ Pup |Min II 13.1. DD Pup |Min II 14.6; Min II - Min I = 0.572P. DE Pup |Min II 12.9. DF Pup |Min II 12.8. DK Pup |Min II 13.0. DM Pup |Min II 13.7; Min II - Min I = 0.62P. DN Pup |Min II 13.5. DO Pup |Min II 13.3. DR Pup |Min II 13.3:. DS Pup |Min II 13.4. DT Pup |Min II 14.3. EK Pup |VB A (B 15", 270deg). P var? Max = 2427747.89 + 2.62587d*E EK Pup |(JD2425500 - 29500) [01343]; since JD2434500 - see Table. EL Pup |P > 1.3d? In the region of the open cluster NGC 2437. EN Pup |Min II 11.4. EQ Pup |Min II 10.9. ES Pup |According to [00412], Max = 2430377 + 187d*E. ES Pup |The elements given in the Table are valid in the interval ES Pup |JD2425600 - 29700. EU Pup |Min II 14.8. FK Pup |A var (P2 = 3000d). Strong SiC2 bands in the spectrum. FM Pup |Min II 14.2. GG Pup |S5/5. GH Pup |VB A (B 10", 195deg; C 16", 280deg; D 14", 315deg). P var. GH Pup |Max = 2425450 + 800d*E (JD2425300 - 28000); since GH Pup |JD2428700 - see Table. Very red. GI Pup |In the region of the open cluster NGC 2437. GK Pup |IN the region of the open cluster NGC 2437. GN Pup |VB A (B 16.5m, 10", 80deg). GP Pup |Min II 13.5. GU Pup |Min II 12.2. GX Pup |Min II 13.9. In the region of the open cluster Cr 173. GY Pup |Min II 12.3. GZ Pup |Min II 12.1. HH Pup |(k - b)2 = 0.14, Delta(S) = 1. HI Pup |Min II 11.0. In the region of the open cluster Cr 173. HK Pup |P var. Max = 2425925.732 + 0.7342532d*E HK Pup |(JD2425300 - 36600) [04127]; since JD2436600 - see Table. HM Pup |There is a shallow Min II. HP Pup |P var? HW Pup |P var? Max = 2429756.28 + 13.4532d*E (JD2427100 - 33000) HW Pup |[03551]; since JD2433000 - see Table. KQ Pup |In the open cluster NGC2422. SB2 (Porb = 9752d [03985]). KT Pup |Min II 13.4. KW Pup |Min II 11.8. KX Pup |Min II 13.04; 0.435P (1930) < Min II - Min I < 0.56P (1973) KX Pup |[03474,08094]; e = 0.15. Apsidal motion. KY Pup |Min II 11.1. LN Pup |Min II 12.9; Min II - Min I = 0.533P. LO Pup |Min II 13.9. LP Pup |d = 0.03P:. LT Pup |Min II 12.6. MN Pup |Min II 13.2. MQ Pup |Min II 9.39. MT Pup |RCB? MW Pup |Min II 9.2. NO Pup |VB A (BC 7.19m V, 8.1". 124deg (delta(M) = 0.0m, 0.20", NO Pup |275deg, NO Pup |1976)). Min II 6.66; Min II - Min I = 0.582P; e = 0.123. NQ Pup |S 4.5/2-. NW Pup |Porb = 1d. NX Pup |Connected with a cometary nebula. OR Pup |In the region of the open cluster NGC 2467. OS Pup |VB A (B 6.10m, 67.4"). OS Pup |In the region of the open cluster C 0812-362. OU Pup |In the region of the open cluster IC 2391. OX Pup |In the region of the open cluster NGC 2451. PS Pup |The depth of Min II 0.028m. PT Pup |P2 = 0.168377d. A (lambda 1550) = 0.043m; PT Pup |0.015m < A(B) < 0.035m. PU Pup |VB (5.2m, 5.6m; 0.11", 43.6deg, 1927). Min II 4.74. PV Pup |VB B (A 6.1m; B 16.9", 340deg; C 10.5m, 100.4", 228deg). PV Pup |Min II 7.31; DII 0.10P; Min II - Min I = 0.47P. PV Pup |The light curve shape in Max and Min II varies. PV Pup |The deviations DB from the mean curve vary from -0.06m PV Pup |to +0.03m with the elements: Max (IDelta(B)I) = PV Pup |2440000.027458 + 1.92207d*E or Max (IDelta(B)I) = PV Pup |2440000.219470 + 0.48003d*E. PW Pup |Min II 9.54; d = 0.095P. In the region of the open PW Pup |cluster NGC 2439. QS Pup |0.008m <= A(u) <= 0.015m. QT Pup |Probably a member of the open cluster NGC 2477. QU Pup |P2 = 0.1680d or 0.2019d; 0.010m <= A(u) <= 0.040m. QV Pup |May be a member of the open cluster NGC 2489. V0360 Pup |Type ACV: is also possible. V0364 Pup |The preceding component of the northern star in the system of two V0364 Pup |CoD-CPD objects, COD-36 3425 and CoD-36 3426 (CPD-36 1171 and CPD-36 V0364 Pup |1172). The cross-identifications of these CoD and CPD objects differ V0364 Pup |from one source to another; our adopted identification is based on the V0364 Pup |paper editions of the catalogs. V0376 Pup |Type ACV: is also possible. V0378 Pup |Type BE is also possible. V0393 Pup |SB, Porb = 2.5248d. V0419 Pup |Not a nearby star (despite having a Gl number). omi Pup |Type EA: is also possible. rho Pup |VB A (B 13.7m, 29.6", 15deg). [Fe/H] = +0.13. P var. rho Pup |Max = 2435552.807 + 0.14088141d*E (JD2413900 - rho Pup |37500) [09756]; Max = 2439887.843 + 0.14088141d*E rho Pup |(JD2439800 - 43700); since JD2444000 - see Table. L 2 Pup |VB A (B 11.5m, 62", 214deg); mu = 0.34", P=18deg. H2O, L 2 Pup |SiO maser. S Pyx |P var. Max = 2411770 + 206.60d*E (JD2405500 - 23700); S Pyx |Max = 2423765 + 207.0d*E (JD2423700 - 29600); S Pyx |since JD2429600 - see Table. T Pyx |Previous outbursts were observed in 1890, 1902, 1920, 1944. RR Pyx |A close companion 14.5m. RZ Pyx |Min II 9.69. SU Pyx |d = 0.016P. TT Pyx |P = 3.031556d? TV Pyx |Depth of Min II 0.05m. TX Pyx |Min II 9.8. TY Pyx |Min II 7.48. TZ Pyx |Min II 11.1. UZ Pyx |VB A (B 7.61m, 110", 180deg). VV Pyx |VB A (B 8.58m, 0.3"). VV Pyx |Range of the variation of combined light is given. VV Pyx |Min II 7.03; DII = 0.08P; Min II - Min I = VV Pyx |0.48P. Min II = 2444622.86709 + 4.5961766d*E. VV Pyx |Apsidal motion (P = 3200 yr). VW Pyx |The nucleus of the planetary nebula K1-2. VW Pyx |The range of the variations of combined light: VW Pyx |15.7 - 17.4 pg. The value of P close to VW Pyx |that found by bond [09767] and the epoch of Max brightness VW Pyx |are given in the Table. R Ret |P var. Max = 2403013 + 280.0d*E (JD2403000 - 13900); R Ret |Max = 2423317 + 276.68d*E (JD2413900 - 25300); R Ret |Max = 2430008 + 279.7d*E (JD2425200 - 30020); R Ret |since JD2430000 - see Table. T Ret |Mean brightness varies with P = 200d. X Ret |(k - b)2 = 0.09. P var. Max = 2427425.47 + 0.4920d*E X Ret |[00357]; Max = 2434334.611 + 0.492011d*E (JD2434300 - 600) X Ret |[00080]; since JD2434600 - see Table. X Ret |The shape of the light curve varies. Blazhko effect: X Ret |Pi >= 45d; 0.13P <= M - m <= 0.23P [00080]. R Sge |P var (70.07d <= P <= 71.24d [09769]. Period variation R Sge |study [00767]. The elements given in the Table are valid R Sge |since JD2434000. The mean brightness varies: R Sge |Min = 2414402 + 1112.d*E [01357]. S Sge |SB1 (Porb = 675d [01358]). P var. Max = 2409863.32 + S Sge |8.381968d*E (JD2406600 - 18000); since S Sge |JD2418000 - see Table. U Sge |VB A (B 9.6m, 92.0", 318deg). Min II 6.71; U Sge |0.014P <= dI <= 0.024P. In the region of the open cluster U Sge |Col 399. Not a member of the cluster. P var [06224,08608]. U Sge |Mean elements are given in the Table representing U Sge |epochs of Min within +-0.008P. The shape of the light U Sge |curve varies. V Sge |VB A (B 13.9m, 9.7", 267deg); SB2 (K1 = 320 km/s, V Sge |K2 = 85 km/s). P var? The depth of eclipses V Sge |varies from 0.6m to 1.3m. The mean brightness outside V Sge |eclipses varies. There are also flares with amplitudes up V Sge |to 3m and small light variations with a time V Sge |scale of minutes, dozens of minutes and a few days. V Sge |spectrum description [03593,09472]. X Sge |VB A (B 13.18m, 6", 248deg). Z Sge |V1 (NGC 6838, M71). Globular cluster member. P var. Z Sge |Max = 2437870 + 175.3d*E (JD2437000 - 38700); since Z Sge |JD2438700 - see Table. RS Sge |The mean brightnese varies: Max = 2435999 + 1124d*E [08104]. RS Sge |Two Algol-like light weakenings were also RS Sge |observed: JD2444837.22, 2444865.17 [09727]. RW Sge |P var. according to [01363] Max = 2424289 + 429d*E. Since RW Sge |JD2434000 - see Table. RZ Sge |Porb ~97m [09771]. Mean cycle is given according to [09785]. RZ Sge |Supermaxima are repeated with the cycle 266d. The period RZ Sge |of superhumps decreases from 101.3m till 100.8m. SY Sge |Min II 10.7. P var. Elements given in the Table are valid SY Sge |in the interval JD2425800 - 38300. TU Sge |d = 0.035P. TX Sge |P var. Max = 2425002 + 155.0d*E (JD2414900 - 25100); TX Sge |since JD2425000 - see Table. UU Sge |VB A (B 16.5m B, 4", 90deg). The nucleus of the planetary UU Sge |nebula Abell 63. Min II 14.41; d = 0.019P. UU Sge |The range of the combined light variation is given. UU Sge |The actual depth of Min I is about 4.3m. Large reflection UU Sge |effect. UZ Sge |Min II 11.6:. P var. Min I = 2429961.231 + 2.215750d*E UZ Sge |(JD2429000 - 41600); since JD2441600 - see Table. VZ Sge |VB A (B 12m, 28.2", 206deg). WY Sge |Nova Sge 1783 (Max JD2372494:). Min I = 2445137.8993 + WY Sge |0.1536342d*E; D = 0.16P. Brightness outside eclipses is WY Sge |usually ~18.7m, the depth of the eclipses is ~ 1.5 - 2m. WY Sge |At present outbursts by 1.6m are sometimes observed WY Sge |similar to the UG type variable outbursts, as well as WY Sge |rapid flickering of light [09708]. WZ Sge |Nova Sge 1913, 1946, 1978. VB A (B 15.76m B, 7", 280deg). WZ Sge |Really it is not a nova. Three outbursts were registered WZ Sge |up to day: JD2420094, 32001, 43844 [09710,09711]. WZ Sge |There are superhumps on the light curve during the WZ Sge |outburst with 0.057250d >= P >= 0.05714d (A=0.3m V) WZ Sge |[09710,09776]. There are light variations between WZ Sge |the outbursts (A = 0.14m - 0.3m). During some of light WZ Sge |weakenings Algol-like eclipses are observed (A = 0.2m) WZ Sge |with the elements: Min I = 2437547.72845 + 0.0566878455d*E WZ Sge |[09774]; D = 0.04P. d = 0.02P. There are also rapid light WZ Sge |oscillations (A <= 0.01m). The periods of these WZ Sge |oscillations before the 1978 outburst were 28.98s and WZ Sge |27.87s [09774], but after this outburst - 28.95963s [09775]. WZ Sge |According to [09777], in 1976 - 78 these oscillations were WZ Sge |represented by the elements: Max = 2443311.790250 + WZ Sge |0.00032254826d*E + 9.8d*10**(-16)*E**2. XY Sge |According to [03705] the spectrum is earlier than M0. AG Sge |P = 117d? BR Sge |d = 0.030P. CP Sge |Min II 13.3. CU Sge |Min II 11.3. CW Sge |Min II 11.7. P var? The shape of the light curve varies. CZ Sge |Min II 15.2. DH Sge |The shape of the light curve varies (1.1m <= A <= 1.7m). DH Sge |P var. Max = 2427612.509 + 0.4695844D*E (JD2427600 - DH Sge |38800) [04027]; since JD2438800 - see Table. DH Sge |Blazhko effect disappeared after the period change DH Sge |(A = 1.1m). DI Sge |P var. Max = 2427929 + 203.0d*E (JD2427500 - 30200) DI Sge |[02641]; since JD2437100 - see Table. DK Sge |Min II 13.0. DL Sge |Min II 11.5. DM Sge |Min II 11.6. DP Sge |P var. Max = 2427985.464 + 0.4883395d*E (JD2427985 - 33000); DP Sge |Max = 2432855.191 + 0.4883339d*E (JD2433000 - 40775); DP Sge |since JD2440775 - see Table. DQ Sge |Min II 14.8. DS Sge |Min II 16.0:. DT Sge |d = 0.05P:. EH Sge |VB A (B 15.6m). EI Sge |Min II 14.6. ER Sge |P var. Max = 2430515.460 + 0.4184209d*E ER Sge |(JD2427000 - 38400); ER Sge |Max = 2438443.388 + 0.4184356d*E (JD2438400 - 41800); ER Sge |since JD2441800 - see Table. FF Sge |d = 0.03P; Min II 13.0. FG Sge |VB A (B 14.2m, 8", 100deg). The central star of the FG Sge |planetry nebula PK 60deg (diameter 36", the age about 6000 FG Sge |years). The brightness of the star steadily increased from FG Sge |13.6 pg in 1894 to the maximum in 1967, and then is FG Sge |steadily decreasing. In 1982 it was 11.0 B. In 1967 the FG Sge |strong absorption lines of rare earth elements appeared FG Sge |in the spectrum. The spectral class steadily becomes FG Sge |later. The signes of new planetary nebula ejection were FG Sge |observed. In 1962 the star entered the instability FG Sge |strip in the Mv, B-V diagram and began to pulsate FG Sge |with a small amplitude and increasing period: Min(V) = FG Sge |2442629 + 59.83d*E + 1.126d*E**2 (JD2442600 - 44530). FG Sge |In twenty years the period increased from 50d to 134d, FG Sge |the amplitude of pulsations changed from 0.2mV to 0.5mV; FG Sge |now it decreased again to 0.2mV, and the period is only FG Sge |90d [09780]. FH Sge |Min II 13.5. FL Sge |There is a close companion 14m. In the minimum probably FL Sge |fainter than 15.9m. FO Sge |P var. Max = 2427578.0 + 67.8d*E (JD2427570 - 28120); FO Sge |Max = 2428134.4 + 72.7d*E (JD2428120 - 30150); FO Sge |since JD2430150 - see Table. FP Sge |Min II 14.9. P = 0.32100275d? FT Sge |P.K.55-1 deg 2. Not a planetary nebula. FU Sge |Min II 15.8. FX Sge |In the region of the globular cluster M71 (NGC 6838). GI Sge |Red. GN Sge |Min II 10.6. GP Sge |Red. GY Sge |P var. Max = 2431264.49 + 51.497d*E (JD2429490 - 34900) GY Sge |[07199]; Max = 2433787.42 + 51.5991d*E (JD2433600 - 37280), GY Sge |Max = 437911.04 + 51.2524d*E (JD2437280 - 40510) [06172]; GY Sge |since JD2444450 - see Table. HH Sge |The cycles 23 - 26d and 300d are observed. HM Sge |VB A (B 14.20m, 10", 182deg). The brightness increased HM Sge |from 17.2m up to 11.3m pg in the interval JD2442280 - HM Sge |42650. Then the light variations in the infrared region HM Sge |appeared with P = 550d [09721,09783] and A(K) = 1.5m. HM Sge |Radio and X-ray source. IR Sge |SF star in a close pair. LN Sge |SF star in a close pair. MV Sge |Possible member of the globular cluster Palomar 10. MZ Sge |Possible member of the globular cluster Palomar 10. PT Sge |P component of a close pair. V0339 Sge |Extremely metal-weak. del Sge |VB A (B, A = 0.04", P = 7 yr); SB2 (Porb = 3725d [09789]). del Sge |The last superior conjunction of the B-star and its del Sge |atmospheric eclipse was in March - April 1980 [09726]. R Sgr |P var. Max = 2405776 + 271.0d*E (JD2399500 - 2407500); R Sgr |Max = 2407115 + 264.2d*E (JD2407100 - 9500); R Sgr |Max = 2418125 + 269.65d*E (JD2409500 - 19500); R Sgr |Max = 2433137 + 267.90d*E (JD2419500 - 36000); R Sgr |since JD2436000 - see Table. S Sgr |P var. Max = 2401029 + 230.6d*E (JD2401000 - 10000); S Sgr |Max = 2411638 + 229.2d*E (JD2410000 - 19500); S Sgr |Max = 2422222 + 232.81d*E (JD2419500 - 27000); S Sgr |since JD2427000 - see Table. T Sgr |Companion F3IV (ro < 0.8"). P var. T Sgr |Max = 2409013 + 385.1d*E (JD2401500 - 10500); T Sgr |Max = 2414582 + 399.0d*E (JD2413000 - 17500); T Sgr |Max = 2424363 + 387.9d*E (JD2417500 - 25500); T Sgr |since JD2425500 - see Table. T Sgr |S 5/6-e. There are Te lines and a very strong T Sgr |Li lambda 6708 line in the spectrum. U Sgr |The member of the open cluster M25 (IC 4725). U Sgr |P var. Max = 2416628.046 + 6.744925d*E (JD2404480 - 30115) U Sgr |[00765]; since JD2430115 - see Table. [A/H] = 0.1. W Sgr |VB A (A 9.2m, 0.116", 153.3deg, 1976.477; B 13.5m, 33.4", W Sgr |233deg; C 13.5m, 47.9", 101deg). P var. W Sgr |Max = 2403198.39 + 7.594695d*E (JD2403100 - 34500); since W Sgr |JD2434500 - see Table. X Sgr |P var. Max = 2410006.22 + 7.01206d*E (JD2403000 - 17000); X Sgr |Max = 2424248.11 + 7.01245d*E (JD2417000 - 34500); since X Sgr |JD2434500 - see Table. Y Sgr |In the region of the open cluster M25 (IC 4725). RR Sgr |P var. Max = 2410008 + 336.0d*E (JD2410000 - 17100) RR Sgr |[09794]; Max = 2422755 + 332.73d*E (JD2422700 - 32100) RR Sgr |[00960]; since JD2432100 - see Table. OH, H2O emission. RS Sgr |VB A (B 9.65m V, 39.0", 86deg). Min II 6.28. RT Sgr |P var. Max = 2412759 + 303.1d*E (JD2412700 - 8300) RT Sgr |[00960]; Max = 2425588 + 308.8d*E (JD2422800 - 26700); RT Sgr |Max = 2428034 + 303.8d*E (JD2426700 - 33500); RT Sgr |since JD2433500 - see Table. RU Sgr |P var. Max = 2413062 + 242.3d*E (JD2410150 - 16700) RU Sgr |[00960]; Max = 2423670 + 242.3d*E (JD2422500 - 24500); RU Sgr |Max = 2428200 + 237.6d*E (JD2424500 - 28800); since RU Sgr |JD2428800 - see Table. RV Sgr |P var. Max = 2411206 + 319.3d*E (JD2410200 - 17000) RV Sgr |[00960]; Max = 2429032 + 321.3d*E (JD2422600 - RV Sgr |29500); since JD2429500 - see Table. RW Sgr |P var. Max = 2413798 + 189.0d*E (JD2413700 - 23000); RW Sgr |Max = 2431998 + 190.87d*E (JD2423000 - 33500); RW Sgr |since JD2433500 - see Table. RX Sgr |P var. Max = 2417730 + 330.3d*E (JD2413000 - 18500); RX Sgr |Max = 2420122 + 346d*E (JD2418500 - 20150); RX Sgr |Max = 2420122 + 323d*E (JD2420100 - 22200); RX Sgr |Max = 2424120 + 345d*E (JD2422200 - 24200); RX Sgr |Max = 2428785 + 332.2d*E (JD2424000 - 31500); RX Sgr |since JD2431500 - see Table. RY Sgr |VB A (B 15.69m, 12"). There are pulsational light RY Sgr |variations (0.1m < A < 1.5m) with the elements: RY Sgr |Max = 2433670 + 38.6056d*E - 78d*10**(-5)*E**2. RY Sgr |light curve [09798,09799]; spectrum description [06261]. ST Sgr |S 6/3-e. SU Sgr |VB A (B 13.5m, 1.0", 240deg, 1932.45). SU Sgr |earlier P = 88d was observed [00017]. SV Sgr |In the nebula M8 (NGC 6523). SW Sgr |P var. Max = 2416338 + 290.3d*E (JD2414000 - 16500); SW Sgr |Max = 2428507 + 288.5d*E (JD2422500 - 29000); SW Sgr |Max = 2429088 + 293.5d*E (JD2429000 - 33000); SW Sgr |since JD2433000 - see Table. SX Sgr |Min II 9.62; d = 0.05P. P var. Min I = 2429114.249 + SX Sgr |4.15395762d*E (JD2410000 - 29150) [00007]; SX Sgr |since JD2429000 - see Table. SY Sgr |In the region of the nebula S188. SZ Sgr |VB A (B 12.5m V, 2.0", 212deg.) VV Sgr |In the region of the open cluster NGC 6494. OH, H2O VV Sgr |emission. VX Sgr |P var; 1m <= A <= 6m. SIO, H2O, OH maser. VX Sgr |Light curve (1935-1969) [06615]. VY Sgr |[A/H] = 0.5. WX Sgr |VB A (B 12.5m, 0.4", 88deg). P var. Min = 2419317.259 + WX Sgr |2.129095d*E (JD2419300 - 24700) [00457]; Min = WX Sgr |2424729.418 + 2.129113d*E (JD2424700 - 39700) WX Sgr |[00279]; since JD2440000 - see Table. WY Sgr |Min II 10.3. WZ Sgr |The member of the open cluster C 1814-190. [A/H] = 0.4. XX Sgr |P var. Max = 2419189.730 + 6.424264d*E (JD2419100 - 30100) XX Sgr |[00637]; since JD2435000 - see Table. XZ Sgr |Min II 8.95; d = 0.022P. P var. Min I = 2420311.519 + XZ Sgr |3.275537d*E (JD2420300 - 28000) [01604]; Min I = XZ Sgr |2436440.137 + 3.27549d*E (JD2428000 - 37500) XZ Sgr |[02516]; Min I = 2441150.348 + 3.2755357d*E XZ Sgr |(JD2437500 - 41500) [07084]; since JD2441500 - see Table. YY Sgr |Min II 10.64; Min II = 2433075.8296 + 2.628463d*E YY Sgr |[02302]. Apsidal motion period is about 300 years. AL Sgr |P var. Max = 2425792 + 79.07d*E (JD2421000 - 26000); AL Sgr |since JD2426000 - see Table. AN Sgr |P var. Max = 2425720 + 339.62d*E (JD2415000 - 26000); AN Sgr |Max = 2428360 + 330.0d*E (JD2426000 - 28500); AN Sgr |since JD2428500 - see Table. AP Sgr |SB? [09004]. AR Sgr |There is a square term in the elements: AR Sgr |-[0.0031d (E-30)**2 + 8.8d]. AS Sgr |Planetary nebula HB6 = 7 + 1deg 1. AU Sgr |In the region of the open cluster and the diffuse nebula AU Sgr |NGC 6514 (M20). AV Sgr |In the region of the open cluster NGC 6546. Not a member AV Sgr |of the cluster. [A/H] = 0.4. P var. AV Sgr |Max = 2429083.30 + 15.4093d*E (JD2421400 - 39100); since AV Sgr |JD2439100 - see Table. AW Sgr |VB A (B 16m, 15", 97deg). AW Sgr |In the region of the open cluster NGC 6546. AY Sgr |[A/H] = 0.2. BB Sgr |VB A (B = V4088 Sgr, 7.49m - 7.87m, 93.5", 102deg). BB Sgr |In the region of the open cluster Cr394. BE Sgr |A var (0.6m <= A <= 1.1m). BM Sgr |P var. BN Sgr |Min II 9.37; d = 0.04P:. BN Sgr |Soft X-ray source. P var [01600]. BQ Sgr |d = 0.017P. P var. Min = 2412592.7905 + 8.01964d*E BQ Sgr |(JD2412590 - 22220) [01696]; since JD2422220 - see Table. CC Sgr |In the region of the globular cluster NGC 6723. CD Sgr |In the region of the globular cluster NGC 6723. P var. CD Sgr |Max = 2416247 + 266.62d*E CD Sgr |(JD2411000 - 23000); since JD2423000 - see Table. CE Sgr |In the region of the globular cluster NGC 6723. CE Sgr |SF component of a close double. CF Sgr |In the region of the globular cluster NGC 6723. CF Sgr |P var. Max = 2415632.81 + 0.570026d*E (JD2411000 - CF Sgr |23800) [01616]; since JD2423900 - see Table. CG Sgr |In the region of the globular cluster NGC 6723. DH Sgr |In the region of the globular cluster NGC 6809 (M55). DI Sgr |In the region of the globular cluster NGC 6809 (M55). DK Sgr |In the region of the globular cluster NGC 6809 (M55). DM Sgr |In the region of the globular cluster NGC 6809 (M55). DO Sgr |In the region of the globular cluster NGC 6809 (M55). DP Sgr |In the region of the globular cluster NGC 6809 (M55). DR Sgr |In the region of the globular cluster NGC 6809 (M55). DS Sgr |In the region of the globular cluster NGC 6809 (M55). DV Sgr |d = 0.044P. EG Sgr |d = 0.010P. FV Sgr |P var. Max = 2424010 + 269.5d*E (JD2424000 - 27500) FV Sgr |[00251]; since JD2427500 - see Table. GG Sgr |P var. Max = 2413840 + 286.5d*E (JD2413800 - 24000); GG Sgr |since JD2424000 - see Table. GK Sgr |According to [05869] - eclipsing. GU Sgr |There are also light variations with <P> = 37.5d, GU Sgr |0.4m <= A(V) <= 1.5m [06273]. HH Sgr |VB (ro = 0.1'). IR Sgr |VB B (A 13.6m; B 10", 220deg). KO Sgr |Similar to UG. It is possible that the observations in Min KO Sgr |brightness refer to a companion. LZ Sgr |VB A (B 16m, 7", 30deg). MV Sgr |Very hot hydrogen deficient extreme helium carbon star. MW Sgr |P var. Max = 2418940 + 202.3d*E (JD2418900 - 23900); MW Sgr |Max = 2428753 + 206.5d*E (JD2423900 - 28950); MW Sgr |since JD2428950 - see Table. NP Sgr |The cycles 100 - 300d are possible. OW Sgr |In the region of the open cluster NGC 6716. V0348 Sgr |VB A (B 15m pg, 16", 73deg). Very hot hydrogen deficient V0348 Sgr |helium carbon star. V0348 Sgr |By the character of light variation and the spectrum the V0348 Sgr |star is unique. The light curve resembling those of RCB V0348 Sgr |type stars is superimposed by conspicuons irregular and V0348 Sgr |semiregular variations with the mean cycle about 200d V0348 Sgr |[02449,09824]. The star is surrounded by a nebula the V0348 Sgr |radius of which equals 1". A fainter nebulous envelope is V0348 Sgr |observed up to 7" from the star. Large infrared V0348 Sgr |excess. Spectrum description [02451,09825]. Probably V0348 Sgr |the star is intermediate between the RCB variables V0348 Sgr |And planetary nebula Wolf-Rayet central stars. V0350 Sgr |SB [09004]. V0354 Sgr |d = 0.02P. V0356 Sgr |Min II 7.24; DII = 0.20P:; d = 0.05P; V0356 Sgr |0.490P (1928) <= Min II - Min I <= 0.505P (1951). V0356 Sgr |Apsidal motion is possible. V0366 Sgr |P var. Max = 2425479.448 + 0.4779616d*E (JD2423990 - 28780) V0366 Sgr |[00705]; since JD2435600 - see Table. [Ca/H] = -0.73. V0367 Sgr |[Ca/H] = -1.21. V0377 Sgr |The epoch of light min is given in the Table. V0377 Sgr |P var. Min = 2426071.24 + 16.17076d*E (JD2425300 - 26600) V0377 Sgr |[00048]; Min = 2427350.25 + 16.19326d*E (JD2426600 - 28700) V0377 Sgr |[01400]; Min = 2436358.98 + 16.1575d*E V0377 Sgr |(JD2436200 - 37300); Min = 2437863.09 + 16.1925d*E V0377 Sgr |(JD2437660 - 39100); Min = 2440114.81 + 16.2407d*E V0377 Sgr |(JD2440200 - 560); since JD2440950 - see Table. V0397 Sgr |There is a square term in the elements: V0397 Sgr |-0.009d*10**(-6)*E**2 V0401 Sgr |Min II 14.1. V0403 Sgr |There is a nonlinear term in the elements: V0403 Sgr |-0.013d*10**(-6)*E**2. V0410 Sgr |VB A (B 13.6m, 270deg). V0426 Sgr |Min II 13.3. V0427 Sgr |There is a nonlinear term in the elements: V0427 Sgr |-131d*10**(-10)*E**2. The shape of the light curve varies: V0427 Sgr |0.17P <= M - m <= 0.22P. V0431 Sgr |Min II 14.9. V0437 Sgr |Min II 14.0. V0440 Sgr |Delta(S) = 9. P var. P = 0.4774659d (JD2416000 - 23000) V0440 Sgr |[00752]; P < 0.4774659d (JD2422000 - 26000) [00235]; V0440 Sgr |Max = 2426581.203 + 0.477474d*E (JD2426000 - 29460) [01000]; V0440 Sgr |since JD2437100 - see Table. V0453 Sgr |There is a nonlinear term in the elements: V0453 Sgr |+0.003d*10**(-6)*E**2. V0457 Sgr |There is a nonlinear term in the elements: V0457 Sgr |-0.005d*10**(-6)*E**2. V0466 Sgr |There is a nonlinear term in the elements: V0466 Sgr |+0.03d*10**(-6)*E**2. V0496 Sgr |Min II 14.3. V0497 Sgr |Min II 16.0. V0505 Sgr |Min II 6.63. P var. Min I = 2433515.3295 + 1.18287141d*E V0505 Sgr |(JD2425500 - 35800) [01642]; Min I = 2437494.4964 + V0505 Sgr |1.1828622d*E (JD2435800 - 37500); Min I = V0505 Sgr |2440055.3991 + 1.1828650d*E (JD2437500 - 40100); V0505 Sgr |Min I = 2442656.5283 + 1.18286917d*E (JD2440100 - V0505 Sgr |42670); since JD2442670 - see Table. The shape of the V0505 Sgr |light curve varies. Deviations from the mean light curve V0505 Sgr |vary with P = 310d. The difference of Min I and Min II V0505 Sgr |depths varies by 0.05m [09830]. V0511 Sgr |P var. Max = 2423950 + 158.8d*E (JD2411300 - 23950); V0511 Sgr |since JD2423950 - see Table. V0515 Sgr |There is a nonlinear term in the elements: +0.015d*E**2. V0519 Sgr |There is a nonlinear term in the elements: +0.0046d*E**2. V0520 Sgr |There is a nonlinear term in the elements: +0.051d*E**2. V0523 Sgr |Min II 9.88. Apsidal motion is observed. In the Table the V0523 Sgr |epoch of Min I is given corresponding to the moment of V0523 Sgr |line of apsides coinciding with the line of sight, when V0523 Sgr |Min II - Min I = 0.50P. The mean period according to V0523 Sgr |[02453] is given; with this period O - C deviations do not V0523 Sgr |exceed +-0.06P for both minima. The period of apsidal V0523 Sgr |motion is 248 years [02453]. Min II - Min I = 0.39P in 1953. V0524 Sgr |Min II 11.2. V0525 Sgr |Min II 8.51. V0526 Sgr |VB A (B 12.40m, 8.6", 7.3deg). Min II 10.20, DII = 0.17P; V0526 Sgr |dI = 0.006P, dII = 0.013P. V0526 Sgr |There are periodic terms in the elements: V0526 Sgr |+0.1369d*sin(0.01295deg*E) - 0.0115d*sin(0.0259deg*E) + V0526 Sgr |0.0011d*sin(0.0388deg*E). Min II = 2422055.0453 + V0526 Sgr |1.919411d*E - 0.1369d*sin(0.01295deg*E) - V0526 Sgr |0.0115d*sin(0.0259deg*E) - 0.0011d*sin(0.0388deg*E). V0526 Sgr |The period of apsidal motion is 146 years. e = 0.224. V0527 Sgr |P var. Max = 2426904.95 + 1.258956d*E (JD2425790 - 7650) V0527 Sgr |[01648]; since JD2438200 - see Table. V0551 Sgr |VB B (A 16.5m; B 12", 135deg). V0552 Sgr |P var. The elements given in the Table are V0552 Sgr |valid since JD2418400. V0554 Sgr |Min II 14.5. V0557 Sgr |P var. Max = 2415110.5 + 16.233d*E (JD2415100 - 22000); V0557 Sgr |Max = 2426100.0 + 16.260d*E (JD2423900 - 27700) [00251]; V0557 Sgr |Max = 2428097.70 + 16.171d*E (JD2427700 - 28800) [00296]; V0557 Sgr |since JD2428800 - see Table. V0558 Sgr |Min II 14.3. V0564 Sgr |P var. Max = 2424056 + 27.8d*E (JD2423780 - 26000) V0564 Sgr |[00251]; Max = 2428403.3 + 27.99d*E (JD2427870 - 29160) V0564 Sgr |[00296]; Max = 2429158.2 + 27.2d (JD2429150 - 515); V0564 Sgr |since JD2429515 - see Table. V0567 Sgr |The central star of the planetary nebula P.K.355 -6deg 1 V0567 Sgr |(M3-21). V0573 Sgr |Min II 12.7. V0574 Sgr |Min II 14.7. V0578 Sgr |According to [02448], Max = 2428710 + 253d*E. V0593 Sgr |P var. Max = 2414150 + 230d*E (JD2414100 - 22900); V0593 Sgr |since JD2423900 - see Table. V0598 Sgr |d = 0.05P. V0611 Sgr |P var. Max = 2414150 + 123d*E (JD2414150 - 19000); V0611 Sgr |since JD2420250 - see Table. V0611 Sgr |The period must probably be doubled because the star V0611 Sgr |resembles RV Tau (Min II 16.2). V0612 Sgr |P var. Max = 2413750 + 107.9d*E (JD2413700 - 17900); V0612 Sgr |since JD2418800 - see Table. V0615 Sgr |P.K.356 -7deg 1 = He 2-349. V0626 Sgr |P var? Max = 2427715.4 + 26.745d*E (JD2425380 - 28800) V0626 Sgr |[00046]; since JD2434500 - see Table. V0631 Sgr |Min II 14.2. V0632 Sgr |P var. Max = 2413350 + 263d*E (JD2413300 - 19000); V0632 Sgr |since JD2420200 - see Table. V0633 Sgr |P var. Max = 2415110 + 224d:*E (JD2415000 - 18800); V0633 Sgr |since JD2420000 - see Table. V0638 Sgr |P var? Max = 2412670 + 73.1d*E (JD2412600 - 14540); V0638 Sgr |since JD2414800 - see Table. V0646 Sgr |P var. Max = 2413350 + 95d*E (JD2413300 - 15900); V0646 Sgr |since JD2423900 - see Table. V0660 Sgr |P var. Max = 2426460 + 235.6d*E (JD2426400 - 35700) V0660 Sgr |[00251]; since JD2435600 - see Table. V0663 Sgr |P var. Max = 2426160 + 305d*E [00251]; V0663 Sgr |since JD2435600 - see Table. V0671 Sgr |P = 292.5d? V0672 Sgr |P var? Max = 2424680 + 228d*E [00251]; since V0672 Sgr |JD2435600 - see Table. V0674 Sgr |P var. Max = 2425830 + 249d*E [00251]; since V0674 Sgr |JD2435600 - see Table. V0675 Sgr |(k - b)2 = -0.01; Delta(S) = 11. V0676 Sgr |P var. Max = 2414140 + 181d*E (JD2414100 - 22600) V0676 Sgr |[00251]; since JD2423900 - see Table. V0679 Sgr |P var. Max = 2415900 + 225d*E (JD2415900 - 22200) V0679 Sgr |[00251]; Max = 2425440 + 223.1d*E (JD2425000 - 29000); V0679 Sgr |since JD2429000 - see Table. V0683 Sgr |Min II 12.5. V0686 Sgr |P var? Max = 2425390 + 225.3d*E [00251]; since V0686 Sgr |JD2435600 - see Table. V0687 Sgr |Min II 12.2. V0691 Sgr |P var? Max = 2426095.550 + 0.46911d*E [00251]; V0691 Sgr |since JD2435630 - see Table. V0703 Sgr |Var 4. According to [02951] the range of light variation, V0703 Sgr |the type of variability and the elements of light V0703 Sgr |variation are erroneously assigned in [01640] to the star V0703 Sgr |Var 3. V0705 Sgr |Min II 12.9. V0710 Sgr |P var. Min = 2426101.550 + 2.3817d*E [00251]; Min = V0710 Sgr |2431286.425 + 2.381633d*E (JD2428390 - 35700) [03513]. V0713 Sgr |P var? Max = 2424680 + 253.4d*E [00251]; since V0713 Sgr |JD2435600 - see Table. V0716 Sgr |P var? Max = 2424670 + 277d*E [00251]; since V0716 Sgr |JD2435600 - see Table. V0718 Sgr |P var? Max = 2425850 + 153.2d*E [00251]; since V0718 Sgr |JD2435600 - see Table. V0721 Sgr |P = 71:d? V0725 Sgr |Unique star. V0725 Sgr |The mean brightness increased from 13.0m to 12.4m V0725 Sgr |since 1889 to 1915, and fell to 12.8m in 1926. From V0725 Sgr |1895 to 1926 real shortperiodic oscillations with the V0725 Sgr |amplitude about 0.4m. In 1928 the amplitude suddenly V0725 Sgr |increased by almost 2m, but the magnitude in maximum V0725 Sgr |remained unchanged. From 1928 to 1935 the light V0725 Sgr |variations became periodic, the period increasing every V0725 Sgr |year by 1d in accordance with the formula: V0725 Sgr |Min = 2426087 + 15.933d*E + 0.0233d*E**2. V0725 Sgr |In 1935 P = 21d. Since 1936 only small oscillations of V0725 Sgr |brightness with a gradual increase of the mean magnitude V0725 Sgr |from 14.3m to 13.9m B (1969). Photoelectric observations V0725 Sgr |in 1968 - 69 reveal the light variations 12.33m - 12.72m V V0725 Sgr |with possible periods 15.4d in 1968 and 45.3d in 1969. In V0725 Sgr |1973 12.28m - 12.58m V, <B-V> = +1.37, P = 50d [07101]. V0727 Sgr |VB A (B = V728 Sgr, 14.7m - 15.9m, 25", 108deg). V0728 Sgr |VB B (A = V727 Sgr, B 25", 108deg). V0734 Sgr |Min II 13.1. V0735 Sgr |VB A (B 15.5m, 6", 315deg). According to B-V, U-B values V0735 Sgr |and spectrum the star is not a UG type variable [09840]. V0738 Sgr |In the region of the globular cluster NGC 6558. V0738 Sgr |According to [05403], RV? P = 86.78d? V0743 Sgr |Min II 14.2. V0745 Sgr |P var. Max = 2416560 + 385.1d*E (JD2411000 - 19260); V0745 Sgr |since JD2419260 - see Table. V0748 Sgr |Min II 14.7; d = 0.04P. V0750 Sgr |d = 0.02P:. V0752 Sgr |Min II 12.7. V0755 Sgr |d = 0.01P. V0757 Sgr |Min II 13.8; d = 0.06P. V0760 Sgr |Min II 13.4. P var. Min = 2414059.5 + 45.10d*E V0760 Sgr |(JD2412800 - 19000); since JD2419000 - see Table. V0761 Sgr |Min II 12.8; d = 0.05P. V0762 Sgr |P var. Max = 2414100 + 461d*E (JD2411000 - 22860); V0762 Sgr |since JD2422860 - see Table. V0763 Sgr |P var. The observations are satisfied by the given V0763 Sgr |elements since JD2415000. V0766 Sgr |d = 0.05P. V0768 Sgr |Min II 13.0. V0770 Sgr |Min II 13.1. V0773 Sgr |[A/H] = 0.1. V0777 Sgr |d = 0.055P. V0778 Sgr |Min II 12.1. V0779 Sgr |Min II 12.0. V0780 Sgr |Min II 12.9; d = 0.08P. V0782 Sgr |d = 0.045P. V0784 Sgr |Min II 12.8. V0786 Sgr |d = 0.025P. V0789 Sgr |In the region of the open cluster Tr 31. V0789 Sgr |P = 5.10470d (Min II 12.7)? [00478]. V0791 Sgr |d = 0.03P:. V0792 Sgr |Min II 12.2. In the region of the open cluster V0792 Sgr |and the diffuse nebula NGC 6514 (M 20). V0793 Sgr |P var. Max = 2412610 + 195d*E (JD2412600 - 19400); V0793 Sgr |since JD2423400 - see Table. V0794 Sgr |P var. Min I = 2413723 + 173.48d*E (JD2413700 - V0794 Sgr |23750); since JD2423750 - see Table. V0801 Sgr |Min II 14.9. V0802 Sgr |[A/H] = -0.4. V0803 Sgr |P = 3.771748d? V0818 Sgr |The shape of the light curve varies. V0819 Sgr |P var? V0824 Sgr |Min II 15.2. V0828 Sgr |There is a close companion. V0838 Sgr |P var? V0839 Sgr |P var? Max = 2426170.126 + 1.835347d*E (JD2425700 - 26600) V0839 Sgr |[01598]; since JD2441500 - see Table. V0841 Sgr |The shape of the light curve varies. V0844 Sgr |P var? V0845 Sgr |Min II 14.6. V0859 Sgr |The shape of the light curve varies. V0879 Sgr |There is a close companion. V0882 Sgr |Min II 14.6. V0884 Sgr |0.20P <= M - m <= 0.40P. Blazhko effect. V0889 Sgr |0.14P <= M - m <= 0.24P. Blazhko effect. V0902 Sgr |Min II 14.8. V0903 Sgr |Min II 13.0. V0919 Sgr |Spectrum description [09845]. V0935 Sgr |P var. Max = 2420040 + 232.0d*E (JD2419500 - 28650); V0935 Sgr |since JD2428600 - see Table. V0938 Sgr |P = 138.27d? V0960 Sgr |nP = 1734d. V0966 Sgr |Min II 14.0. V0977 Sgr |d = 0.03P. V0981 Sgr |Min II 14.8. V0985 Sgr |Min II 14.3. V0986 Sgr |d = 0.015P. V0993 Sgr |dI = 0.05P:; Min II 13.7, DII = 0.09P, dII = 0.00P. V0994 Sgr |Min II 12.8:. V0998 Sgr |The depth of Min II 0.04m:. V1000 Sgr |Min II 13.9. V1002 Sgr |Min II 13.7. V1004 Sgr |[A/H] = -0.2. V1005 Sgr |Min II 13.9. V1013 Sgr |Min II 15.0. V1017 Sgr |VB B (A 10.6m V; B 15", 270deg). V1017 Sgr |For a long time the star was considered to be a recurrent V1017 Sgr |nova. Three considerable flares were observed: in 1901 V1017 Sgr |(10.8m), 1919 (6.2m), and 1973 (10.5m). Composite spectrum V1017 Sgr |with a trace of a hot component [03872]. V1023 Sgr |In the region of the open cluster Cr 394. Min II 13.0:. V1026 Sgr |Min II 13.4. V1028 Sgr |Min II 14.4. V1032 Sgr |Min II 15.0. V1033 Sgr |The shape of the light curve varies. Blazhko effect? V1034 Sgr |d = 0.025P:. V1049 Sgr |Min II 13.6; Min II - Min I = 0.326P; DII = 0.025P. V1050 Sgr |Min II 14.1. V1056 Sgr |Min II 14.1. V1063 Sgr |The shape of the light curve strongly varies. Blazhko V1063 Sgr |effect? V1068 Sgr |Min II 15.4. V1069 Sgr |The shape of the light curve strongly varies. Blazhko V1069 Sgr |effect? V1071 Sgr |P = 1.3560996d? V1072 Sgr |The shape of the light curve strongly varies. Blazhko V1072 Sgr |effect? V1080 Sgr |P var. The shape of the light curve varies. V1081 Sgr |P var? V1089 Sgr |Cycle <= 30d. V1100 Sgr |d = 0.02P:. V1108 Sgr |Min II 11.9; Min II - Min I = 0.516P. V1109 Sgr |Min II 14.5. V1127 Sgr |There is a nonlinear term in the elements: V1127 Sgr |+78.10d**(-10)*E**2. V1136 Sgr |d = 0.020P. V1148 Sgr |In the region of the globular cluster NGC 6553. V1153 Sgr |P var? Max = 2428391.266 + 1.332624d*E (JD2427680 - V1153 Sgr |30910); since JD2435630 - see Table. V1177 Sgr |Min II 11.4. V1178 Sgr |d = 0.03P:. V1180 Sgr |[A/H] = -0.4. V1181 Sgr |[A/H] = 0.6. P var. Max = 2428452.25 + 21.341d*E V1181 Sgr |(JD2427400 - 31000) [01638]; since JD2433000 - see Table. V1185 Sgr |[A/H] = -0.5. P var. Max = 2428778.86 + 13.9123d*E V1185 Sgr |(JD2427500 - 32750) [01638]; Max = 2437485.4 + V1185 Sgr |13.901345d*E (JD2437100 - 43760) [08519]; V1185 Sgr |since JD2444000 - see Table. V1187 Sgr |[A/H] = -0.8. V1188 Sgr |[CA/H] = -0.37. V1189 Sgr |[A/H] = -1.1. V1190 Sgr |P = 3.000078d? V1191 Sgr |Min II 14.4. V1205 Sgr |The alternative period is possible: 0.659820d [01638]. V1209 Sgr |A var. V1211 Sgr |Delta(S) = 3:. V1214 Sgr |There is a nonlinear term in the elements: V1214 Sgr |-0.25d*10**(-7)*E**2. V1216 Sgr |mu = 0.720", P = 106.7deg. V1223 Sgr |As a rule has a persistent high state; five drops by two V1223 Sgr |to more than three magnitudes have been registered and a V1223 Sgr |twelve year interval of irregular variations at V1223 Sgr |intermediate magnitudes. According to [09850] there are V1223 Sgr |slow variations in brightness by 0.15m on a time scale V1223 Sgr |of ~1 day. They are superimposed by variations with the V1223 Sgr |orbital period P orb (Max = 2444749.9866 + 0.140239d*E) V1223 Sgr |and with amplitude up to 0.15m. These variations in their V1223 Sgr |turn are superimposed by the others: with P = 794.38s V1223 Sgr |and the amplitude from 0.03m up to 0.15m V1223 Sgr |(Max = 2444750.00404 + 0.009194215d*E and (sometimes) with V1223 Sgr |P = 849.8s and a twice smaller amplitude V1223 Sgr |(Max = 2444750.00350 + 0.00983588d*E). Besides there are V1223 Sgr |rapid brightness variations on time scales 10 - 100s by V1223 Sgr |0.10m - 0.20m, and high frequency flickering by 0.05m. V1223 Sgr |According to [09851], the period of X-ray pulses associated V1223 Sgr |with the rotation of the compact object is 12.5 minutes. V1276 Sgr |Min II 14.3. V1280 Sgr |Brightness of Max varies by 2m with the period 5230d. V1281 Sgr |The light variation is not strictly periodic. V1282 Sgr |P var. Min = 2427651.297 + 1.754574d*E (JD2427650 - V1282 Sgr |30560) [00705]; since JD2435600 - see Table. V1284 Sgr |Min II 13.5. EB? V1287 Sgr |Var 3. According to [02951] the range of light variation of V1287 Sgr |Var 4 (V703 Sgr), the type of variability and the elements V1287 Sgr |of light variation of Var 4 (V703) are erroneously V1287 Sgr |assigned in [01640] to the star Var 3. V1287 Sgr |According to [02951] the range of light variation, the type V1287 Sgr |of variability and the elements of light variation are V1287 Sgr |erroneously assigned in [01640] to the star Var 4. V1287 Sgr |Min II 14.8. V1290 Sgr |[A/H] = -1.2. V1303 Sgr |[A/H] = -0.8. P var? Max = 2438241.176 + 18.46812d*E V1303 Sgr |(JD2427700 - 38250) [00001]; since JD2444000 - see Table. V1304 Sgr |[A/H] = 0.3. P var. Max = 2428758.10 + 12.9287d*E V1304 Sgr |(JD2427590 - 28820) [01640]; since JD2435600 - see Table. V1309 Sgr |Not far from V4032 Sgr. V1311 Sgr |V 14 in the globular cluster NGC 6656 (M22). V1311 Sgr |Not a member of the cluster. V1312 Sgr |P var? Max = 2428815.600 + 0.6011427d*E (JD2427590 - 28820) V1312 Sgr |[01640]; since JD2435630 - see Table. V1314 Sgr |P var? Max = 2428346.536 + 0.657489d*E (JD2427600 - V1314 Sgr |28820) [01640]; since JD2435630 - see Table. V1317 Sgr |P var? V1327 Sgr |SR?, L? [08424]. V1328 Sgr |P = 0.39937d? V1329 Sgr |VB B (A 17.2m; B 1.4", 120deg). P var. Max = 2432388.777 + V1329 Sgr |0.48306d*E (JD2431670 - 32740) [03524]; V1329 Sgr |since JD2443300 - see Table. V1331 Sgr |Min II 16.5. V1352 Sgr |P var. Max = 2431998.851 + 0.49505d*E (JD2431670 - V1352 Sgr |33150) [01680]; Max = 2443341.844 + 0.49493d*E V1352 Sgr |(JD2443300 - 350); Max = 2444087.558 + 0.49516d*E V1352 Sgr |(JD2444050 - 110); in the interval JD2444400 - 410 - see V1352 Sgr |Table. V1356 Sgr |Min II 18.0:. V1357 Sgr |Min II 19.0. V1359 Sgr |P var? V1369 Sgr |P var. Max = 2432736.821 + 0.52956d*E (JD2431670 - 33150) V1369 Sgr |[03524]; since JD2440700 - see Table. V1374 Sgr |Delta(S) = 1. V1378 Sgr |Delta(S) = -3:. V1387 Sgr |Delta(S) = 3. V1389 Sgr |The epoch of Min brightness is given. V1390 Sgr |Min II 17.6. V1392 Sgr |P var. Max = 2432739.791 + 0.55032d*E (JD2431670 - 33150) V1392 Sgr |[03524]; since JD2440700 - see Table. V1393 Sgr |Delta(S) = 3. V1394 Sgr |Min II 18.0. V1401 Sgr |The epoch of Min brightness is given. V1405 Sgr |P var. Max = 2432031.778 + 0.46511d*E (JD2431670 - 33150) V1405 Sgr |[06094]; since JD2443300 - see Table. V1408 Sgr |A var (0.5m <= A <= 1.4m). V1409 Sgr |P var. Max = 2432739.822 + 0.65159d*E (JD2431670 - 33150) V1409 Sgr |[03524]; since JD2443300 - see Table. V1412 Sgr |The epoch of Min brightness is given. V1415 Sgr |P var? V1416 Sgr |Delta(S) = 3. P var? Max = 2432002.875 + 0.42767d*E V1416 Sgr |(JD2431670 - 33150) [06094]; since JD2440700 - see Table. V1418 Sgr |P var. Max = 2432740.818 + 0.45423d*E (JD2431670 - 33150) V1418 Sgr |[03524]; since JD2440700 - see Table. V1419 Sgr |P var. Max = 2432061.669 + 0.57144d*E (JD2431670 - 33150) V1419 Sgr |[01680]; since JD2440700 - see Table. V1425 Sgr |Min II 18.8. V1426 Sgr |Delta(S) = 1.5. V1429 Sgr |The epoch of Min brightness is given. V1435 Sgr |Min II 18.0; Min II - Min I = 0.53P. V1437 Sgr |V8 (NGC 6522); not a member of the globular cluster. V1438 Sgr |V9 (NGC 6522); not a member of the globular cluster. V1439 Sgr |P = 0.53711d? [06094]. V1443 Sgr |Min II 18.6. V1446 Sgr |Min II 18.0. V1447 Sgr |Min II 18.2. V1454 Sgr |Min II 15.4. V1457 Sgr |Min II 19.0. V1459 Sgr |The depth of Min II is 0.04m. V1460 Sgr |P var. Max = 2432067 + 162.0d*E (JD2431670 - 33150) V1460 Sgr |[01680]; since JD2440340 - see Table. V1464 Sgr |Delta(S) = 1. V1465 Sgr |P var. Max = 2431702.660 + 0.45757d*E (JD2431700 - 940); V1465 Sgr |Max = 2432706.945 + 0.45757d*E (JD2431940 - 32740) [03524]; V1465 Sgr |since JD2440740 - see Table. V1466 Sgr |The epoch of Min brightness is given. V1473 Sgr |According to [08424] P = 340d. V1487 Sgr |Min II 18.8. V1491 Sgr |Min II 18.5. V1498 Sgr |SP component of a close pair. P var. V1498 Sgr |Max = 2432739.728 + 0.47467d*E (JD2431670 - 33150) [06094]; V1498 Sgr |since JD2443300 - see Table. V1508 Sgr |VB. V1509 Sgr |Min II 18.1:. V1510 Sgr |According to [06094], P = 0.48546d. V1516 Sgr |P var? Max = 2432740.753 + 0.49709d*E (JD2431670 - V1516 Sgr |33150) [03524]; since JD2440700 - see Table. V1517 Sgr |P < 2.0d. V1523 Sgr |P var? Max = 2432417.702 + 0.36202d*E (JD2431670 - 33150) V1523 Sgr |[03524]; since JD2443300 - see Table. V1526 Sgr |Min II 18.3. V1537 Sgr |Min II 17.4; Min II - Min I = 0.54P. V1540 Sgr |According to [08424], P = 465d. V1546 Sgr |The epoch of Min brightness is given. V1550 Sgr |P = 0.37432d? [06094]. V1554 Sgr |Min II 17.5. V1557 Sgr |Delta(S) = 8. V1558 Sgr |Delta(S) = 1. V1559 Sgr |The depth of MinII is 0.04m. V1561 Sgr |Min II 17.7. V1567 Sgr |Min II 18.0. V1569 Sgr |Min II 18.6. V1576 Sgr |[Ca/H] = -1.23. V1577 Sgr |P var. Max = 2426200 + 290d*E (JD2426000 - 30560) V1577 Sgr |[02449]; since JD2430560 - see Table. V1580 Sgr |P var (310d <= P <= 365d). V1589 Sgr |[Ca/H] = -0.91. V1602 Sgr |d = 0.03P. V1610 Sgr |P < 0.5d. V1639 Sgr |The shape of the light curve varies. V1640 Sgr |(k -b)2 = 0.24. P var? V1642 Sgr |250d <= P <= 350d. V1643 Sgr |Min II 12.1. According to [05771], RR?, P = 0.34d. V1644 Sgr |The shape of the light curve varies. V1647 Sgr |VB A (B 9.13m, 8", 104deg). Min II 7.43, DII = 0.059P, V1647 Sgr |Min II - Min I = 0.262P (JD2441830); V1647 Sgr |Min II = 2441830.55561 + 3.28282227d*E. V1647 Sgr |The apsidal motion period is 592.5 +- 6.5 years. V1648 Sgr |Close VB. Flat Min. V1652 Sgr |Close VB. Flat Min. V1653 Sgr |Close VB. Flat Min. V1656 Sgr |Close VB. Flat Min. V1658 Sgr |P var.Max = 2426560 + 105d*E (JD2417000 - 28000) V1658 Sgr |[00842]; since JD2428000 - see Table. V1660 Sgr |Close VB. Flat Min. V1661 Sgr |Close VB. Flat Min. P var. Max = 2426850 + 275d*E V1661 Sgr |(JD2424000 - 26850); since JD2436700 - see Table. V1667 Sgr |P var. Max = 2426560 + 158d*E (JD2417000 - 36000) V1667 Sgr |[00842]; since JD2436000 - see Table. V1668 Sgr |Close VB. Flat Min. V1670 Sgr |A var. P var. The shape of the light curve varies V1670 Sgr |(probably with a period of about 11 years). V1675 Sgr |A possible companion of 16m. V1679 Sgr |Close VB. Flat Min. V1681 Sgr |A possible companion of 16m. V1690 Sgr |A possible companion of 16m. V1691 Sgr |Close VB. Flat Min. V1691 Sgr |P var. Max = 2426520 + 235d*E (JD2417000 - 28000) V1691 Sgr |[00842]; since JD2436000 - see Table. V1697 Sgr |A possible companion of 16m. V1698 Sgr |A possible companion of 16m. V1699 Sgr |P var. Max = 2425410 + 203.6d*E (JD2417000 - 27600) V1699 Sgr |[00842]; since JD2436000 - see Table. V1703 Sgr |A possible companion of 16m. V1705 Sgr |P var. Max = 2425860 + 142d*E (JD2417000 - 27000) V1705 Sgr |[00842]; since JD2435800 - see Table. V1711 Sgr |[A/H] = -1.1. P var. Max = 2435365.19 + 30.46d*E V1711 Sgr |(JD2432700 - 35400) [02570]; since JD2442200 - see Table. V1714 Sgr |In the region of the open cluster Ruprecht 134. V1721 Sgr |d = 0.03P:. V1723 Sgr |Min II 13.8. V1730 Sgr |Min II 14.8:; d = 0.03P:. V1741 Sgr |In the nebula and the cluster NGC 6530 (M8). Var1. V1743 Sgr |In the nebula and the cluster NGC 6530 (M8). Var2. V1747 Sgr |In the nebula and the cluster NGC 6530 (M8). Var3. V1748 Sgr |In the nebula and the cluster NGC 6530 (M8). Var4. V1749 Sgr |In the nebula and the cluster NGC 6530 (M8). Var6. V1750 Sgr |In the nebula and the cluster NGC 6530 (M8). Var8. V1751 Sgr |In the nebula and the cluster NGC 6530 (M8). Var7. V1752 Sgr |In the nebula and the cluster NGC 6530 (M8). Var13. V1753 Sgr |In the nebula and the cluster NGC 6530 (M8). Var14. V1755 Sgr |In the nebula and the cluster NGC 6530 (M8). Var15. V1758 Sgr |In the nebula and the cluster NGC 6530 (M8). Var16. V1761 Sgr |In the nebula and the cluster NGC 6530 (M8). Var19. V1762 Sgr |In the nebula and the cluster NGC 6530 (M8). Var20. V1764 Sgr |In the nebula and the cluster NGC 6530 (M8). Var23. V1765 Sgr |In the nebula and the cluster NGC 6530 (M8). Var24. V1768 Sgr |In the nebula and the cluster NGC 6530 (M8). Var26. V1769 Sgr |In the nebula and the cluster NGC 6530 (M8). Var27. V1771 Sgr |In the nebula and the cluster NGC 6530 (M8). Var29. V1772 Sgr |In the nebula and the cluster NGC 6530 (M8). Var28. V1773 Sgr |In the nebula and the cluster NGC 6530 (M8). Var31. V1774 Sgr |In the nebula and the cluster NGC 6530 (M8). Var30. V1775 Sgr |In the nebula and the cluster NGC 6530 (M8). Var33. V1776 Sgr |In the nebula and the cluster NGC 6530 (M8). Var36. V1777 Sgr |In the nebula and the cluster NGC 6530 (M8). Var37. V1778 Sgr |In the nebula and the cluster NGC 6530 (M8). Var34. V1779 Sgr |In the nebula and the cluster NGC 6530 (M8). Var40. V1780 Sgr |In the nebula and the cluster NGC 6530 (M8). Var39. V1781 Sgr |In the nebula and the cluster NGC 6530 (M8). Var41. V1782 Sgr |In the nebula and the cluster NGC 6530 (M8). Var44. V1784 Sgr |In the nebula and the cluster NGC 6530 (M8). Var45. V1785 Sgr |In the nebula and the cluster NGC 6530 (M8). Var46. V1786 Sgr |In the nebula and the cluster NGC 6530 (M8). Var48. V1787 Sgr |In the nebula and the cluster NGC 6530 (M8). Var47. V1788 Sgr |In the nebula and the cluster NGC 6530 (M8). Var50. V1789 Sgr |In the nebula and the cluster NGC 6530 (M8). Var51. V1790 Sgr |In the nebula and the cluster NGC 6530 (M8). Var49. V1790 Sgr |Western component of a close pair. V1791 Sgr |In the nebula and the cluster NGC 6530 (M8). Var53. V1792 Sgr |In the nebula and the cluster NGC 6530 (M8). Var55. V1793 Sgr |In the nebula and the cluster NGC 6530 (M8). Var54. V1794 Sgr |In the nebula and the cluster NGC 6530 (M8). Var56. V1795 Sgr |In the nebula and the cluster NGC 6530 (M8). Var58. V1797 Sgr |In the nebula and the cluster NGC 6530 (M8). Var59. V1798 Sgr |In the nebula and the cluster NGC 6530 (M8). Var60. V1800 Sgr |In the nebula and the cluster NGC 6530 (M8). Var61. V1801 Sgr |In the nebula and the cluster NGC 6530 (M8). Var62. V1802 Sgr |In the nebula and the cluster NGC 6530 (M8). Var63. V1803 Sgr |In the nebula and the cluster NGC 6530 (M8). Var64. V1803 Sgr |SP component of a close pair. V1805 Sgr |In the nebula and the cluster NGC 6530 (M8). Var66. V1807 Sgr |In the nebula and the cluster NGC 6530 (M8). Var67. V1808 Sgr |In the nebula and the cluster NGC 6530 (M8). Var68. V1828 Sgr |P var. Max = 2424402 + 12.985d*E (JD2423800 - 36000) V1828 Sgr |[02515]; since JD2436000 - see Table. V1831 Sgr |P var. Max = 2428849.4 + 26.58d*E (JD2427500 - 31270) V1831 Sgr |[02447]; since JD2435630 - see Table. V1843 Sgr |P = 163.7d? [05869]. V1845 Sgr |Flat Min. Close companion? V1864 Sgr |Epoch of light maximum is given. V1869 Sgr |P var. Max = 2434178 + 346d*E (JD2427590 - 34220) V1869 Sgr |[02447]; since JD2435630 - see Table. V1882 Sgr |The shape of the light curve varies. V1891 Sgr |A companion of 16m. V1894 Sgr |V4 (NGC 6637). Possible member of the globular cluster V1894 Sgr |NGC 6637 (M 69). V1895 Sgr |P var. Max = 2421065 + 156.0d*E (JD2418850 - 21100); V1895 Sgr |since JD2427600 - see Table. V1900 Sgr |A companion of 15m. V1904 Sgr |A companion of 15m. V1911 Sgr |P var. Max = 2428832.4 + 10.0581d*E (JD2427600 - 34220) V1911 Sgr |[02447]; since JD2435630 - see Table. The shape of the V1911 Sgr |light curve varies? V1925 Sgr |P var? V1942 Sgr |In the region of the open cluster Ruprecht 147. V1945 Sgr |In the region of the open cluster and the diffuse nebula V1945 Sgr |NGC 6514 (M20). V1946 Sgr |In the region of the open cluster and the diffuse nebula V1946 Sgr |NGC 6514 (M20). V1947 Sgr |In the region of the open cluster and the diffuse nebula V1947 Sgr |NGC 6514 (M20). All the published charts V1947 Sgr |for this variable are wrong. According to [09861] the V1947 Sgr |star actually lies 1.1 mm south and 0.8 mm east of V1947 Sgr |"D2" in fugure 3 published in [02428]. V1948 Sgr |In the region of the open cluster and the diffuse nebula V1948 Sgr |NGC 6514 (M20). V1949 Sgr |In the region of the open cluster and the diffuse nebula V1949 Sgr |NGC 6514 (M20). V1950 Sgr |In the region of the open cluster and the diffuse nebula V1950 Sgr |NGC 6514 (M20). V1951 Sgr |In the region of the open cluster and the diffuse nebula V1951 Sgr |NGC 6514 (M20). V1954 Sgr |VB(ro = 2"). P var. V1954 Sgr |There is a nonlinear term in the elements: V1954 Sgr |-4.1313d*10**(-8)*E**2. V1958 Sgr |Min II 14.0. V1962 Sgr |In the region of the open cluster and the V1962 Sgr |diffuse nebula NGC 6618 (M 17). V1963 Sgr |In the region of the open cluster and the diffuse nebula V1963 Sgr |NGC 6618 (M 17). V1966 Sgr |In the region of the open cluster and the diffuse nebula V1966 Sgr |NGC 6618 (M 17). V1969 Sgr |There are three close faint companions (15.8m-16.3m). V1970 Sgr |In the region of the open cluster and the diffuse nebula V1970 Sgr |NGC 6618 (M 17). V1971 Sgr |In the region of the open cluster and the diffuse nebula V1971 Sgr |NGC 6618 (M 17). V1973 Sgr |In the region of the open cluster and the diffuse nebula V1973 Sgr |NGC 6618 (M 17). V1975 Sgr |In the region of the open cluster and the diffuse nebula V1975 Sgr |NGC 6618 (M 17). The presence of a blue companion is V1975 Sgr |possible. V1976 Sgr |In the region of the open cluster and the diffuse nebula V1976 Sgr |NGC 6618 (M 17). V1977 Sgr |In the region of the open cluster and the diffuse nebula V1977 Sgr |NGC 6618 (M 17). V1980 Sgr |Min II 11.7; DII = 0.11P; Min II - Min I = 0.52P. V1996 Sgr |VB. V2003 Sgr |S 5.5/5. In the region of the open cluster M 25 (IC 4725). V2007 Sgr |V 26 (NGC 6656 = M 22). V2008 Sgr |P = 120 - 135d. V2028 Sgr |In the region of the globular cluster NGC 6681 (M 70). V2037 Sgr |A close companion is possible. V2054 Sgr |P > 450d? V2064 Sgr |VB. Combined brightness of the star and the close V2064 Sgr |companion was estimated. It is not clear which star is V2064 Sgr |variable. V2065 Sgr |NP component of a close binary. V2094 Sgr |P < 0.5d. V2106 Sgr |VB. Combined brightness of the components was estimated. V2148 Sgr |VB. Combined brightness of the components was estimated. V2148 Sgr |The variable is the northern component. V2276 Sgr |P < 30d. V2282 Sgr |Star L. In the region of the open cluster and the diffuse V2282 Sgr |nebula NGC 6514 (M20). Late spectrum. V2283 Sgr |Min II 10.59:. Apsidal motion with P = 560 years [07107]: V2283 Sgr |0.739P (1898) <= Min II - Min I <= 0.797P (1965). V2283 Sgr |There are periodic terms in the V2283 Sgr |elements given in the Table: V2283 Sgr |+0.5414d*sin(0.006deg*(E + 45019)) - 0.0995d*sin(0.012deg* V2283 Sgr |(E + 45019)) + 0.0217d*sin(0.018deg*(E + 45019)); Min II = V2283 Sgr |2438946.7619 + 3.4714231d*E - 0.5414d*sin(0.006deg* V2283 Sgr |(E + 45019)) - 0.0995d*sin(0.012deg*(E + 45019)) - 0.0217d* V2283 Sgr |sin(0.018deg*(E + 45019)). V2284 Sgr |P var. V2285 Sgr |In the region of the globular cluster NGC 6558. V2313 Sgr |Min II 16.8. V2315 Sgr |P = 0.193d? V2323 Sgr |Blue [08424]. V2341 Sgr |The epoch of Min brightness is given. V2342 Sgr |V 17 (NGC 6626 = M28). V2342 Sgr |The member of this globular cluster. Min II 13.5. V2343 Sgr |A close companion of 14.5m. V2346 Sgr |Cycles 50 - 100d. V2349 Sgr |Min II 9.2. V2351 Sgr |Min II 10.31. V2352 Sgr |P var. There is a nonlinear term in the elements: V2352 Sgr |0.0525d*E**2. V2355 Sgr |In the region of the globular cluster NGC 6637 (M 69). V2358 Sgr |In the region of the globular cluster NGC 6642. V2359 Sgr |In the region of the globular cluster NGC 6637 (M 69). V2360 Sgr |In the region of the globular cluster NGC 6637 (M 69). V2361 Sgr |In the region of the globular cluster NGC 6637 (M 69). V2362 Sgr |A close companion of 15m. V2366 Sgr |P var. There is a nonlinear term in the elements: V2366 Sgr |+0.6815d*10**(-9)*E**2. V2367 Sgr |V28 (NGC 6656 = M22). Not a member of this globular cluster. V2367 Sgr |P = 323d? V2378 Sgr |Two close companions of 15.3m and 15.8m. V2389 Sgr |P var? V2391 Sgr |P = 189d? V2413 Sgr |P var. The elements are valid in the interval V2413 Sgr |JD2425440 - 30905. V2416 Sgr |P.K. 7 +1G 2. V2425 Sgr |E? V2442 Sgr |P = 0.5d? V2449 Sgr |Min II 17.4. V2468 Sgr |Blue [08424]. V2471 Sgr |VB B (A 14.6m; B 8", 225deg). V2493 Sgr |Blue [08424]. V2506 Sgr |P.K. 3 -4deg 6. V2507 Sgr |Min II 14.6. V2508 Sgr |Min II 14.1:. V2509 Sgr |Min II 7.50. V2510 Sgr |The epoch of Min brigtness is given. The elements given V2510 Sgr |in the Table are valid since JD2427440. V2520 Sgr |VB. V2526 Sgr |The epoch of Min brightness is given. V2526 Sgr |P var. Min = 2428699.5 + 31.3224d*E (JD2424100 - 31400) V2526 Sgr |[05590]. Since JD2431400 - see Table. V2529 Sgr |Min II 14.5. Twice shorter period is given in [05590]. V2540 Sgr |P var. V2544 Sgr |VB? V2552 Sgr |VB A (B 15.7m). V2553 Sgr |There are two close companions. V2562 Sgr |Northern component of a close pair. The companion is of V2562 Sgr |16m. V2563 Sgr |P var. V2564 Sgr |P var? V2565 Sgr |VB B (A 12.5m; B 90deg). V2566 Sgr |P var. [Ca/H] = -0.52. V2567 Sgr |[Ca/H] = -0.57. V2568 Sgr |P var? V2576 Sgr |P var. Max = 2426200 + 149d*E (JD2423500 - 27000); V2576 Sgr |since JD2433000 - see Table. V2577 Sgr |P var? V2578 Sgr |VB. In the region of the globular cluster NGC 6642. V2579 Sgr |P var. Max = 2429926.251 + 0.5911903d*E (JD2427590 - V2579 Sgr |34200) [05590]; since JD2435600 - see Table. V2584 Sgr |P var. Max = 2426564.347 + 0.534829d*E (JD2423940 - V2584 Sgr |33860); since JD2437820 - see Table. V2592 Sgr |In the region of the globular cluster NGC 6656 (M22). V2593 Sgr |P var. Max = 2428780.349 + 0.5123825d*E V2593 Sgr |(JD2427680 - 34200) [05590]; since JD2435600 - see Table. V2594 Sgr |P var. V2598 Sgr |A companion 15.8m. Spectrum description [06495]. V2601 Sgr |P.K. 12 -7deg 1. The epoch of Min brightness is given. V2616 Sgr |Min II 13.0. V2617 Sgr |Min II 9.63. V2620 Sgr |P = 185.6d? V2625 Sgr |P = 0.75837d? V2628 Sgr |P = 171d:?/205d:?/256d:?. V2645 Sgr |P var? V2649 Sgr |P = 143d:? V2672 Sgr |P = 196.8d? /204.5d, /255.3d? /315.0d? V2682 Sgr |P = 228.5d? V2687 Sgr |P = 174d:? V2703 Sgr |P = 270d:? V2719 Sgr |SR? V2731 Sgr |P = 147d:? V2732 Sgr |P = 188.6d? V2733 Sgr |P = 244d:? V2736 Sgr |[Ca/H] = -1.45. V2738 Sgr |[Ca/H] = -0.67. V2740 Sgr |P = 269.0d? V2745 Sgr |[Ca/H] = -1.15. V2756 Sgr |P.K. 2 -5deg 1. The epoch of Min brightness is given. V2763 Sgr |P = 216d:? V2777 Sgr |[Ca/H] = -0.83. V2783 Sgr |P = 265.0d? V2789 Sgr |P = 255.5d? V2798 Sgr |P = 244.5d? V2816 Sgr |P = 250d:? V2828 Sgr |P = 0.39669d? V2830 Sgr |Cepheid? V2833 Sgr |P = 224.0d? V2834 Sgr |P = 275d:? V2846 Sgr |P = 0.39659d? V2868 Sgr |P = 235.5d? V2876 Sgr |Min II 15.7:. V2877 Sgr |P = 254.5d? V2893 Sgr |P = 250d:? V2900 Sgr |P = 0.49835d? V2905 Sgr |Spectrum description [04452,06495]. V2918 Sgr |P = 197d:? V2937 Sgr |[Ca/H] = -0.75. V2947 Sgr |RV Tau? Cepheid? V2959 Sgr |P = 0.37233d? V2962 Sgr |P = 209.5d? V2967 Sgr |P = 0.68750d? V2988 Sgr |P = 213.0d? The coordinates given in [05869] are erroneous. V2996 Sgr |RV Tau? Cepheid? V3004 Sgr |[Ca/H] = -0.76. V3005 Sgr |RV Tau? Cepheid? V3016 Sgr |P var? V3032 Sgr |P = 153d:? V3033 Sgr |The coordinates given in [05869] are erroneous. V3034 Sgr |P = 154d:? V3038 Sgr |P = 252d:? V3052 Sgr |RV Tau? Cepheid? V3062 Sgr |EW? P = 0.59610d? V3065 Sgr |P = 179.8d?/215.5d? V3071 Sgr |P = 291d:? V3072 Sgr |P = 194d:? V3088 Sgr |P = 215d:? V3105 Sgr |[Ca/H] = -0.82. V3106 Sgr |P = 261d:? V3111 Sgr |P = 182.8d? V3127 Sgr |UG? Not red. V3128 Sgr |Nova? Only one Max was observed. V3170 Sgr |[Ca/H] = -0.82. V3175 Sgr |P = 179.8d? V3176 Sgr |P = 197d:? V3179 Sgr |P = 297d:? V3186 Sgr |[Ca/H] = -1.28. V3190 Sgr |P = 227.0d? V3196 Sgr |RV Tau? Cepheid? V3207 Sgr |P = 237d:? V3239 Sgr |P = 226d:? V3249 Sgr |UG? V3285 Sgr |P = 173.8d /196.2d? V3294 Sgr |P = 121d:? /177d:? V3295 Sgr |P = 197d:? V3335 Sgr |RV Tau? Cepheid? V3353 Sgr |P var? V3356 Sgr |P = 239.5d? V3365 Sgr |P = 197d:? /252d:? V3388 Sgr |P = 125d:? /160d:? V3395 Sgr |P = 159d:? V3412 Sgr |Cepheid? V3433 Sgr |P = 287.0d? V3443 Sgr |P = 177.6d? V3444 Sgr |P = 160d:? V3459 Sgr |P var. The shape of the light curve varies. V3467 Sgr |RV Tau? Cepheid? V3473 Sgr |SR? V3500 Sgr |RV Tau? Cepheid? V3501 Sgr |Min II 15.7:. V3508 Sgr |The member of the open cluster M25 (IC 4725). V3511 Sgr |RV Tau? Cepheid? V3536 Sgr |P = 239.5d? V3537 Sgr |P = 318.0d? V3551 Sgr |P = 165.2d? /201.0d? V3560 Sgr |P = 181d:? V3564 Sgr |Cepheid? V3566 Sgr |P = 249.0d? V3583 Sgr |P = 228.0d? V3588 Sgr |[Ca/H] = -0.69. V3625 Sgr |P = 294d:? V3634 Sgr |P = 145d:? V3645 Sgr |In the region of the open cluster M25 (IC 4725). V3709 Sgr |P = 240.0d? V3718 Sgr |P var. There is a nonlinear term V3718 Sgr |in the elements: +0.865d*10**(-10)*E**2. V3748 Sgr |P = 0.305327d? V3765 Sgr |[Ca/H] = -0.78. V3783 Sgr |In the region of the globular cluster NGC 6681 (M70). V3784 Sgr |P = 176.4d? V3788 Sgr |In the region of the globular cluster NGC 6723. Red. V3791 Sgr |In the region of the open cluster and the diffuse nebula V3791 Sgr |NGC 6514 (M20). V3792 Sgr |VB A (B 8.92m, 13.3", 90deg). Min II 6.81. V3792 Sgr |The range of the combined light variation is given in the V3792 Sgr |Table. The shape of the light curve varies. V3804 Sgr |Spectrum description [06495,07099]. V3811 Sgr |P2 = 4d? Spectrum description [07099,09845]. V3817 Sgr |VB A (B 16m). V3819 Sgr |P var. There is a nonlinear term in the elements: V3819 Sgr |+10**(-10)*E**2. V3829 Sgr |A close companion. V3832 Sgr |A close companion. V3834 Sgr |Cepheid or eclipsing? V3837 Sgr |P = 0.565d? [06383]. V3838 Sgr |VB A (B 15.8m). V3841 Sgr |P var. Max = 2431970 + 358d*E (JD2423900 - 33000); V3841 Sgr |since JD2433000 - see Table. V3842 Sgr |A close companion with M2? Spectral class possibly exists. V3843 Sgr |In the region of the globular cluster NGC 6642. V3853 Sgr |V22 (NGC 6656 = M22). The member of this globular cluster. V3855 Sgr |V31 (NGC 6656 = M22). Possible member of the cluster. V3857 Sgr |According to [06278] the spectral class is M8. V3867 Sgr |Under the chart S 4903 is printed erroneously instead of V3867 Sgr |CSV 4309. V3868 Sgr |P var. Max = 2426130 + 270d*E (JD2423900 - 33900); V3868 Sgr |since JD2435700 - see Table. V3874 Sgr |P var. Max = 2436035 + 115.3d*E (JD2426000 - 38000); V3874 Sgr |since JD2438000 - see Table. V3875 Sgr |P var. P = 358d (JD2424000 - 33800); since V3875 Sgr |JD2435000 - see Table. V3876 Sgr |P var. Max = 2430090 + 345d*E (JD2423900 - 32000); V3876 Sgr |Max = 2436830 + 358d*E (JD2436000 - 41500) [06279]; V3876 Sgr |since JD2441400 - see Table. V3879 Sgr |VB (Delta(m) = 2.6m, ro = 0.6"). V3880 Sgr |OH, SiO, H2O maser. V3885 Sgr |Porb = 0.206d [04939]. V3885 Sgr |Besides the irregular variability high-frequency V3885 Sgr |oscillations are sometimes observed with V3885 Sgr |P1 = 29.0s, P2 = 30.15s and with amplitudes of 0.00028m. V3885 Sgr |In the spectrum there are extremely broad absorption V3885 Sgr |lines of HI and HeI. The Balmer lines have emission V3885 Sgr |components. X-ray source. V3886 Sgr |Type EB? V3893 Sgr |Connected with a ring nebula. V3894 Sgr |Min II 6.37. P var? V3899 Sgr |In the region of the open cluster and the diffuse nebula V3899 Sgr |NGC 6514 (M20). V3900 Sgr |V7 (NGC 6522). Not a member of this globular cluster. V3903 Sgr |The member of the open cluster Collinder 367. V3903 Sgr |In the nebula Simeis 188. V3907 Sgr |The epoch of Min brightness is given. V3929 Sgr |P.K.5 -5deg 2. V3961 Sgr |SB1 (Porb = 690d [09915]). V4024 Sgr |SB. V4032 Sgr |Not far from V1309 Sgr. V4034 Sgr |Flat Min. Close companion? V4046 Sgr |Flares (11.1m - 12.4m U). V4048 Sgr |Min II 12.6; DII = 0.15P. V4051 Sgr |In the region of the globular cluster NGC 6638. V4051 Sgr |Not a member of the cluster. V4052 Sgr |In the region of the globular cluster NGC 6638. V4052 Sgr |Not a member of the cluster. V4054 Sgr |In the region of the globular cluster NGC 6638. V4054 Sgr |Not a member of the cluster. V4055 Sgr |In the region of the globular cluster NGC 6638. V4055 Sgr |Not a member of the cluster. V4058 Sgr |d = 0.02P V4060 Sgr |P var. Max = 2437846 + 283d*E (JD2436030 - 38970); V4060 Sgr |since JD2438970 - see Table. V4066 Sgr |d ~0.07P. V4067 Sgr |V32 (NGC 6656 = M22). V4067 Sgr |Not a member of the globular cluster. V4068 Sgr |V17 (NGC 6656 = M22). V4068 Sgr |Not a member of the globular cluster. V4069 Sgr |V33 (NGC 6656 = M22). V4069 Sgr |Not a member of the globular cluster. V4390 Sgr |SB2 and speckle binary. V4417 Sgr |The variability may be due to the fainter (B) component. V4429 Sgr |A giant, according to HIPPARCOS data, despite the published V4429 Sgr |luminosity class (V). V4955 Sgr |Close to the N of V4521 Sgr, the periods differ considerably. V5099 Sgr |SU UMa-type cv. V5112 Sgr |A symmetrical minimum lasted for several months, with variations also outside it. eta Sgr |VB A (B 8.0m, 3.5",105deg); mu alpha = -0.0107s, eta Sgr |mu delta = -0.166". mu Sgr |VB A (B 10.48m, 16.9", 285deg; C 13.0m, 25.2", 119deg; mu Sgr |D 9.69m, 48.5", 312deg; E 9.25m, 50.0", 115deg). SB2 mu Sgr |(e = 0.4). The variability type is EA/GS + ACYG. mu Sgr |According to [09922] there are also quasiperiodical light mu Sgr |variations with the amplitudes 0.08m - 0.15m and cycles mu Sgr |from 16d to 40d. ups Sgr |Min II 4.59. R Sco |V7 (NGC 6093 = M80). Probable field star. R Sco |P var. Max = 2400518 + 220.2d*E (JD2400500 - 04000) R Sco |[00960]; Max = 2404493 + 225.86d*E (JD2404000 - 08600); R Sco |Max = 2409003 + 222.29d*E (JD2408600 - 33300); since R Sco |JD2433300 - see Table. S Sco |V6 (NGC 6093 = M80). Cluster non-member. S Sco |P var. Max = 2400986 + 177.00d*E (JD2400900 - 17500); S Sco |since JD2417500 - see Table. T Sco |4.0" N, 2.7" E from the center of the globular cluster T Sco |NGC 6093 = M80. U Sco |Previous outbursts: U Sco |2401646: (1863), 2417343 (1906), 2428342 (1936). Y Sco |Since 1972 varies its brightness in the range 12.3m-15.0m Y Sco |irregularly, maxima are unpredictable [08080]. Z Sco |P var. Max = 2425546 + 357.17d*E (JD2412500 - Z Sco |25600); since JD2430000 - see Table. RR Sco |SiO maser. P var. Max = 2416944 + 284.31d*E RR Sco |(JD2411000 - 18000); Max = 2422828 + 278.09d*E RR Sco |(JD2422800 - 40000); since JD2440000 - see Table. RU Sco |P var. During JD2425000 - 40000 - see Table. RV Sco |VB A (B 13.0m, 5.9", 325deg). RW Sco |OH, H2O, SiO maser. RY Sco |P var, nonlinear term: +4.10d*10**(-6)*E**2. [A/H] = 0.2. RY Sco |VB A (B 10.70m, F8:, 13.8", 220.5deg, 1965; RY Sco |C 11.5m, 2.0", 102deg, 1964; D 11.43m, 24", 80deg). RY Sco |Combined brightness of AC is given. RZ Sco |P var. Max = 2413994 + 161.20d*E (JD2413600 - 22700); RZ Sco |Max = 2422858 + 155.79d*E (JD2422700 - 28000); RZ Sco |Max = 2428156 + 160.29d*E (JD2428000 - 35000); since RZ Sco |JD2437500 - see Table. SV Sco |P var. Max = 2418886 + 258.5d:*E (JD2411600 - 19000); SV Sco |Max = 2424233 + 252.43d*E (JD2420500 - 28600); SV Sco |Max = 2429055 + 255.9d:*E (JD2428600 - 35000); SV Sco |since JD2437000 - see Table. SY Sco |In the region of the open cluster NGC 6475 = M7. TX Sco |In the region of the open cluster NGC 6475 = M7. TX Sco |Probable cluster member. XX Sco |The elements Max = 2413786 + 152d*E XX Sco |[00031] do not represent the observations from [09447]. AC Sco |According to [00266], CST:, 12.2m - 12.6m pg. AH Sco |OH, H2O, SiO maser. AI Sco |P2 = 966.6d. AL Sco |Min II 11.3. AN Sco |EA type is possible. AP Sco |The chart in [09447] is wrong. AR Sco |According to [07104], T Tau type spectrum. AU Sco |VB A (B = V725 Sco, 0.4', 0deg). AV Sco |The chart and data in [09447] correspond to another star. BI Sco |VB B (A = GW Sco; B 6", 150deg). BM Sco |In the region of the open cluster NGC 6405 = M6. BN Sco |In the region of the open cluster NGC 6475 = M7. BN Sco |Resembles R Cen. BS Sco |d <= 0.03P. According to [00021], SP F8. BT Sco |P var. There is periodic term in the elements given in the BT Sco |Table: +0.05d*sin(176deg + 0.0857deg*E). Blazhko effect? BV Sco |Doubtful identification in [09447]. CF Sco |Min II 13.8. CK Sco |VB A (B 15m, 14"). CL Sco |The brightness in optical and UV range is modulated CL Sco |according to the elements: Min (pg) = 2427020 + 624.7d*E. CL Sco |Outbursts 1892, 1899, 1907, 1926. CP Sco |N /= 4. CQ Sco |[A/H] = -1.4. DX Sco |VB A (B p). EZ Sco |VB A (B 15.6m nf). FQ Sco |VB A (B 16m vis). FU Sco |VB A (B np). Min II 12.7, Min II - MiN I = 0.493P. FV Sco |d = 0.015P. Depth of Min II 0.1m pg. FY Sco |VB A (B 15m, 15", 35deg). GG Sco |VB A (B 15m, 8", 45deg). GM Sco |The nothern one of the two stars noted on the chart for GM Sco |SVS 1677. GW Sco |VB A (B = BI Sco, 6", 150deg). IU Sco |VB A (B 16.4m nf). IU Sco |Max = 2413280 + 69.05d*E (1893 - 1906); IU Sco |during 1910 - 1928 - see Table. KO Sco |Rapid variations: A = 1.0m. Slow changes: KO Sco |A = 0.5m, P = 2000d +-. KQ Sco |[A/H] = +0.3. P var? LO Sco |P var? Before JD2419150 Max = 2411500 + 450d*E; LO Sco |since JD2423900 - see Table. LO Sco |The spectrum is later than M5. LR Sco |The spectrum resembles RCrB in Max light [08090]. LR Sco |IR excess. RCB type minima were not observed. OO Sco |In the region of the open cluster TR 29. OQ Sco |The chart in [06286] is wrong. QZ Sco |P var. Before JD2420400 Max = 2412640 + 158d*E; QZ Sco |since JD2423900 - see Table. V0347 Sco |P var. Before JD2418700 Max = 2411500 + 198d*E; V0347 Sco |since JD2423900 - see Table. V0381 Sco |d = 0.046P. V0382 Sco |In the region of the open cluster NGC 6475 = M7. V0385 Sco |In the region of the open cluster CR 338. V0387 Sco |Min II 12.2. V0390 Sco |P var. Before JD2422500 Max = 2420330 + 466d*E; V0390 Sco |since JD2423900 - see Table. V0393 Sco |Min II 8.3. V0400 Sco |Min II 15.0. V0402 Sco |In the region of the open cluster NGC 6475 = M7. V0403 Sco |d ~0.02P. The depth of Min II 0.05m. V0407 Sco |In the region of the open cluster NGC 6475 = M7. V0411 Sco |Min II 14.0. V0412 Sco |Min II 14.8. In the region of the open cluster V0412 Sco |NGC 6475 = M7. V0420 Sco |In the region of the open cluster NGC 6475 = M7. V0421 Sco |P var. Before JD2418000 Max = 2413830 + 293d*E; V0421 Sco |since JD2423900 - see Table. V0423 Sco |Min II 14.2. In the region of the open cluster V0423 Sco |NGC 6475 = M7. V0425 Sco |In the region of the open cluster NGC 6475 = M7. V0426 Sco |In the region of the open cluster NGC 6475 = M7. V0429 Sco |In the region of the open cluster NGC 6475 = M7. V0430 Sco |In the region of the open cluster Tr 30. V0432 Sco |In the region of the open cluster Tr 30. V0437 Sco |d = 0.02P. Min II 13.9. V0439 Sco |P var. Before JD2418200 Max = 2413350 + 166.5d*E; V0439 Sco |since JD2419900 - see Table. V0440 Sco |In the region of the open cluster Tr 30. V0446 Sco |P var? before JD2435000 Max = 2434980.1 + V0446 Sco |28.6195d. [A/H] = -1.0. V0450 Sco |A = 0.9m pg. V0453 Sco |VB A (B 13.51m, F7V, 13.5", 168deg). Min II 6.70. V0453 Sco |The light curve shape var? V0455 Sco |P.K.351deg + 3deg1. Planetary nebula nature is doubtful. V0455 Sco |Nova-like outbursts separated by several years. V0457 Sco |Min II 11.3. V0460 Sco |d = 0.02P. V0464 Sco |d = 0.03P. V0466 Sco |Min II 13.7. V0467 Sco |P var. P = 2.41354d (1889 - 1903); since 1903 - see Table. V0470 Sco |[A/H] = 0.1. V0471 Sco |Min II 15.2, dII = 0.08P(!). V0472 Sco |d = 0.02P. V0474 Sco |Min II 10.6. V0483 Sco |CI = +3.5m. V0485 Sco |Short term variations are superimposed. V0486 Sco |D >= 4d? P = 1d is possible. In the region of V0486 Sco |the open cluster NGC 6383. V0487 Sco |[Fe/H] = -1.67, Delta(S) = 9.0. V0490 Sco |Min II 12.5. V0491 Sco |Min II 13.2. V0494 Sco |A var (1.27m - 1.66m B). P var? Delta(S) = 2. V0494 Sco |VB A (B 12.72m y, 23"). V0495 Sco |Short term variation are superimposed. V0495 Sco |(Delta(m)short = 0.5m +-). V0496 Sco |In the region of the open cluster NGC 6414. V0496 Sco |d = 0.03P. V0497 Sco |Min II 13.6. V0499 Sco |AII = 0.47m V. Min I - Min II = 0.504P. V0502 Sco |In the region of the open cluster C 1712 - 407. V0507 Sco |The epoch of Max from [00300] contradicts the elements. V0540 Sco |VB A (B 15.2m sp). V0547 Sco |VB B (A 14.2m sf). V0549 Sco |[A/H] = -1.1. V0555 Sco |[A/H] = -0.3. V0562 Sco |Min II 12.1. V0566 Sco |d = 0.01P:. V0567 Sco |VB A (B 13.01m, 10"sp, CD 30"nf). P var. V0568 Sco |d = 0.04P. V0569 Sco |Min II 11.4. V0570 Sco |P var? Unusually broad Max. V0573 Sco |d = 0.06P. In the region of the open cluster Tr 24. V0574 Sco |In the region of the open cluster Tr 24. V0575 Sco |Min II 12.4. V0579 Sco |In the region of the open cluster Tr 24. V0581 Sco |Min II 11.9. V0584 Sco |Min II 13.1. V0585 Sco |d = 0.03P:. V0586 Sco |d = 0.04P. In the region of the open cluster Tr 24. V0588 Sco |d = 0.02P. In the region of the open cluster Tr 24. V0589 Sco |d = 0.05P. In the region of the open cluster Tr 24. V0590 Sco |In the region of the open cluster NGC 6231. V0592 Sco |Min II 13.3. V0593 Sco |d = 0.05P:. V0594 Sco |d = 0.01P. V0603 Sco |d = 0.04P. V0606 Sco |d = 0.07P. V0607 Sco |Min II 10.3. V0609 Sco |Min II 13.7. V0611 Sco |d = 0.04P. Min II 13.7. V0612 Sco |d = 0.05P. V0613 Sco |d = 0.04P. V0616 Sco |Min II 12.4. V0619 Sco |Min II 12.1. V0620 Sco |d = 0.02P. V0621 Sco |d = 0.04P. V0622 Sco |Min II 14.2. V0623 Sco |Long intervals in Max without changes, sometimes becomes V0623 Sco |faint. V0625 Sco |VB A (B 13.2m sf). Min II 13.5. V0627 Sco |Min II 14.1. V0628 Sco |Min II 12.4. V0629 Sco |Apsidal motion. V0631 Sco |Min II 13.2. V0632 Sco |d = 0.06P. V0633 Sco |Min II 12.2. V0634 Sco |Min II 12.2. V0636 Sco |SB1 (Porb = 1318d). V0638 Sco |d = 0.07P. V0640 Sco |Min II 13.5. V0656 Sco |The chart in [06286] is wrong. V0660 Sco |VB A (B 16.0m s). V0672 Sco |P = 180d is possible. V0674 Sco |VB A (B 15.0m s). V0677 Sco |The chart in [06286] is wrong. V0679 Sco |P = 364d is possible. V0690 Sco |VB A (B 14.40m y, 6", 0deg). The range of the combined V0690 Sco |light is given. Delta(S) = 4. V0698 Sco |D <= 0.20d, d = 0.043d. V0700 Sco |Min II 10.3. V0701 Sco |Min II 9.05. P var. Min I = 2439329.6657 + 0.76187133d*E V0701 Sco |(JD2428000 - 39400) [07177]; since JD2439400 - see Table. V0701 Sco |Probable member of the open cluster NGC 6383. V0702 Sco |Probable member of the open cluster NGC 6383. V0703 Sco |P0 = 0.1499615d [03521]; P1 - see Table V0703 Sco |(P var?). Also noted P = 0.04162025d [03521]. V0703 Sco |A var (0.23m - 0.46m). Beat phenomenon: V0703 Sco |Max = 2436760.249 + 0.497306d*E [03521]. Delta(S) = 1. V0703 Sco |In the region of the open cluster NGC 6405 = M6. V0705 Sco |Min II 14.1:. V0706 Sco |Moments of Max from [00046] contradict the tabulated V0706 Sco |elements. According to [04678], A <= 0.05m V V0706 Sco |during 6 nights. V0708 Sco |In the region of the open cluster NGC 6475 = M7. V0709 Sco |IN the region of the open cluster NGC 6475 = M7. V0709 Sco |[A/H] = -0.6. V0710 Sco |Min II 14.2. V0711 Sco |In the region of the open cluster NGC 6475 = M7. V0712 Sco |Min II 14.0. V0714 Sco |d = 0.05P:. P may be twice longer. V0717 Sco |[A/H] = 0.9. V0718 Sco |D ~4d. Another Min 2429847 - 849 [00270]. V0720 Sco |In the region of the open cluster NGC 6475 = M7. V0723 Sco |In the region of the open cluster NGC 6475 = M7. At the V0723 Sco |edge of a dark cloud. V0725 Sco |VB B (A = AU Sco, B 0.4', 0deg). V0729 Sco |Possibly a Nova. V0732 Sco |P may be twice longer. V0733 Sco |Possibly a Nova. V0734 Sco |Possibly a Nova. V0735 Sco |The light curve shape var. V0738 Sco |d = 0.04P:; Min II 13.4:. In the region of the open V0738 Sco |cluster NGC 6475 = M7. V0740 Sco |In the region of the open cluster NGC 6475 = M7. V0741 Sco |There is a red variable close to the coordinates in the V0741 Sco |discovery announcement [02448], but a different star is V0741 Sco |marked in the chart in [02448]. V0749 Sco |P = 410d is possible. V0756 Sco |Min II 10.7. V0760 Sco |dI = 0.02P; Min II 7.4; DII = 0.2P:, dII = 0.03P. V0761 Sco |IN type is not excluded. V0764 Sco |Min II 9.0. V0805 Sco |Possibly P is twice shorter. V0818 Sco |Sco X-1. SB. V0818 Sco |Var X-ray and multi-component radio source. V0818 Sco |Lx/Lbol = 300 - 1000. The epoch of Min is V0818 Sco |given for the periodic component of the light variation V0818 Sco |(A ~0.25m). Flickering and flares up to 1m with V0818 Sco |time scale from dozens of seconds to minutes. The V0818 Sco |mean brightness level decreased in the middle of V0818 Sco |1960-es by 0.3m-0.4m. The spectrum with blue continuum V0818 Sco |and H, HeI, HeII, CIII, NIII emissions. V0819 Sco |Min II 13.2. V0821 Sco |Min II 14.5. V0822 Sco |VB? Combined brightness. V0827 Sco |Min II 14.1. V0833 Sco |Min II 11.2. V0837 Sco |d ~0.03P:; Min II 14.3. V0838 Sco |Min II 13.4. V0842 Sco |Min II 12.3. V0843 Sco |Min II 10.5. V0848 Sco |Min II 13.1. RRC type with twice shorter period is V0848 Sco |possible. V0849 Sco |Min II 14.1. V0853 Sco |d = 0.05P; Min II 14.1. V0856 Sco |VB C (A = BS 6000, 6.65m, AO-3III; B 12.55m, 16", V0856 Sco |298deg; C 44", 185deg; D 11.7m, CD 1.3", 105deg, 1945). V0857 Sco |Erroneously labelled "10" (instead of "11") in the chart. V0858 Sco |Erroneously labelled "11" (instead of "10") in the chart. V0861 Sco |SB1. Min II 6.28. Depths of minima var. In the region of V0861 Sco |the open cluster NGC 6231, Cr 316, Tr 24. V0862 Sco |Usually 6.67m - 6.76m. A flare of 40m duration on July 3, V0862 Sco |1965. In the region of the open cluster NGC 6405 = M6. V0866 Sco |VB (Delta(m) ~0.5m, ~1", 200deg). m (6370 A) = V0866 Sco |11.14m - 12.37m. IR excess. V0870 Sco |B-V = +3.38m - +3.52m. In the region of the open cluster V0870 Sco |NGC 6231. V0877 Sco |Min II 13.1. V0883 Sco |VB A (B 12.60m, 9", 130deg). P var? V0883 Sco |Min = 2438228.315 + 1.294745d*E (JD2438200 - 40500) V0883 Sco |[06871]; since JD2440500 - see Table. Deep Min II. V0884 Sco |4U 1700-37. LX/Lbol = 0.00007. V0884 Sco |Eclipsing X-ray source. Eclipse duration is variable V0884 Sco |in the ranges 0.61d <= dx <= 1.10d. The epoch of the V0884 Sco |middle of the X-ray eclipse coinciding with Min II is V0884 Sco |given. X-ray flux var in the scale from seconds till V0884 Sco |hours. Sometimes a periodic modulation with P ~97 V0884 Sco |Min is present, its amplitude in the optical band reaches V0884 Sco |Delta(V) ~0.01m. Min II 6.57; Min I - Min II = 0.63P, V0884 Sco |dI=0.2P. Surrounded by the ring nebula Sh 2. in the region V0884 Sco |of the open cluster NGC 6281. Field star. V0885 Sco |Noticeable Min II. V0889 Sco |The northern component of a triple. V0890 Sco |VB A (B 11.5m, 0.5' n). V0894 Sco |A = 0.6m pg. V0896 Sco |Co-ordinates or the chart may be erroneous. V0900 Sco |In the region of the open cluster NGC 6231. V0900 Sco |The light curve is a sinusoidal wave. Possibly V0900 Sco |P = 6.20d; 6.85d. V0903 Sco |N96 [02448]. Erroneously identified with V479 Sco. V0906 Sco |In the region of the open cluster NGC 6475 = M7. Probable V0906 Sco |cluster member. VB (delta(mV) = 0.8m, 0.1", 111deg, 1957). V0906 Sco |The range of the combined light variation is given. V0906 Sco |Min II 6.21. V0907 Sco |In the region of the open cluster NGC 6475 = M7. V0907 Sco |Min II 9.2. V0911 Sco |Alternative P = 4.2d. V0913 Sco |Alternative P = 0.976d. IR excess. V0914 Sco |VB (delta(mV) = 2m, 3", 200deg). Sine wave with P = 2.69d, V0914 Sco |Delta(B) = 0.15m (B = 12.91m) [09753]. V0915 Sco |VB A (B 10.43m, WN6, 14", 330deg; C 11.40m, 20", 202deg; V0915 Sco |D 13.96m, 22", 80deg, 1973). The brightness decreased from V0915 Sco |6.32m to 6.50m during JD2443680 - 44115. V0917 Sco |VB A (B 17m: sp). The outburst: rise 1930-1936, V0917 Sco |Max 1936-1938, decline 1938-1952. V0919 Sco |In the region of the open cluster NGC 6231. V0920 Sco |In the region of the open cluster NGC 6231. Multiple V0920 Sco |periodicity: P1 - see Table, semiamplitude A1 = 0.0051m; V0920 Sco |P2 = 0.10765d. A2 = 0.0046m; P3 = 0.10388d, A3 = 0.00485m; V0920 Sco |P4 = 0.12137d, A4 = 0.0036m; P5 = 0.6929d?, A5 = 0.0028m. V0921 Sco |The star illuminates a nebula. V0922 Sco |Multiple periodicity, superposition of frequencies with V0922 Sco |amplitudes 0.0010m - 0.0352m. V0923 Sco |D = 0.32d:. The elements need confirmation. In the region V0923 Sco |of the open cluster NGC 6281. V0924 Sco |B-V var: +1.90, +2.50, V0924 Sco |Light fluctuations by 0.1m - 0.2m (u, b) in several V0924 Sco |minutes. V0925 Sco |VB A (B ~10", faint, blue). Probable member of the open V0925 Sco |cluster TR 27. In Vr possible values of P: 105.3d, 73.0d, V0925 Sco |188.7d, 312.5d [09950]. V0926 Sco |3U 1735-44 = Sco XR-3. Bursts superimpose small light V0926 Sco |variations with P = 0.18d which is apparently the V0926 Sco |orbital period [04394]. V0927 Sco |The epoch of Min in U light is given. IR excess. alf Sco |ADS 10074 A(B 5.1m, B4Ve, A = 2.9", Porb = 878 yr.). alf Sco |Connected with a nebula. zet 1 Sco |In the region of the open cluster NGC 6231. kap Sco |SB. P2 = 0.205430d. P1 var. Beat phenomenon: kap Sco |Pi = 7.3316d. lam Sco |SB1. Porb = 5.6d? Apuls = 0.02m. Long period light changes: lam Sco |Max = 2440376.15 + 10.1605d*E [09761]. One eclipse was lam Sco |found (JD2440690, A ~0.04m) [06388]. mu 1 Sco |Min II 3.12. sig Sco |VB AA (A 5.5m, 0.37", 96deg, 1981, sig Sco |orbital motion?; B 8.45m, B9.5V, 20.1", 273deg, sig Sco |1961); SB1, Porb = 33.06d. P0 var. sig Sco |Max Vr = 2420000.1465 + 0.24682815d*E (1918 - 1924) sig Sco |[09953]; Max = 2432306.918 + 0.246846d*E (JD2432000 - 37800) sig Sco |[09764]; since JD2437800 - see Table. sig Sco |A0 = 0.036m y. P1 = 0.2396674d, A1 = 0.013m y [09762]. sig Sco |Pbeat = 8.256d = Porb/4 [09957]. sig Sco |Connected with a nebula. R Scl |VB A (B 19.9m, 10", 234deg). CO emission. S Scl |P var. Max = 412774 + 367.9d*E (JD2405400 - 20500); S Scl |Max = 2423035 + 360.6d*E (JD2421250 - 27740); S Scl |Max = 2427738 + 370.4d*E (JD2427700 - 34000) [00960]; S Scl |Since JD2434000 - see Table. H2O emission. T Scl |P var. Max = 2417400 + 202.26d*E (JD2411300 - 19000); T Scl |Max = 2420390 + 197.85d*E (JD2419000 - 23600); T Scl |since JD2423600 - see Table. V Scl |P var. Max = 2414006 + 294.8d*E (JD2411600 - 18200); V Scl |Max = 2422866 + 297.2d*E (JD2420400 - 35100); V Scl |since JD2435100 - see Table. X Scl |P var. Max = 2413796 + 258.7d*E (JD2413500 - 22800); X Scl |since JD2422800 - see Table. Y Scl |The cycles 100d: and 300d: are sometimes observed. RT Scl |Min II 10.47. [Fe/H] = -0.75. P var. There is RT Scl |a nonlinear term in the elements given in the Table: RT Scl |-9.04d*10**(-11)*E**2. RU Scl |(k - b)2 = 0.09. A var [03429]. P var. Max = 2425094.4175 + RU Scl |0.4933257d*E (JD2416750 - 25100) [00183]; Max = RU Scl |2427403.177 + 0.4933239d*E (JD2425100 - 30650) RU Scl |[01381]; since JD2430650 - see Table. RW Scl |P var? SV Scl |[Fe/H] = -1.82. P var? Max = 2439468.364 + SV Scl |0.3773636d*E (JD2427300 - 39500) [05233]; SV Scl |since JD2439850 - see Table. SY Scl |H2O maser. P var? Max = 2426160 + 411d*E [00193]; since SY Scl |JD2440400 - see Table. SZ Scl |Min II 13.68. UY Scl |Near the galaxy NGC 55. UZ Scl |VB A (B 15.81m, 23", 135deg); (k - b)2 = 0.14. The UZ Scl |shape of the light curve varies. VV Scl |Min II 8.50. ACV? [08083]. VY Scl |Porb = 0.1662d? [09932]. High and low states of the VY Scl |system are observed. VZ Scl |High and low states of the system are observed [09933]. WZ Scl |There are two oscillations with the periods P1 and WZ Scl |P2: P1 = 0.06576d, P2 = 0.095944d, P1/P2 = 0.6854. XX Scl |There are two oscillations with the periods P1 and XX Scl |P2: P1 = 0.048898d, P2 = 0.051350d, P1/P2 = 0.95225. AI Scl |There are two oscillations with the periods P1 and AI Scl |P2: P1 = 0.044d, P2 = 0.0931d, P1/P2 = 0.47. AL Scl |Min II 6.20; Min II - Min I = 0.475P; DII = 0.08P. AO Scl |mu = 0.46", P = 187deg. BC Scl |May be eclipsing. BI Scl |Type E: is also possible. R Sct |[Fe/H] = -1. P var. Min I = 2377165 + 142.8d*E R Sct |(JD2377160 - 9820); Min I = 2384885 + 142.6d*E R Sct |(JD2384890 - 8170); Min I = 2394451 + 141.4d*E R Sct |(JD2394450 - 8500); Min I = 2398777 + 142.4d*E R Sct |(JD2398770 - 2404320); Min I = 2404627 + 137.4d*E R Sct |(JD2404600 - 6410); Min I = 2406561 + 142.7d*E R Sct |(JD2406560 - 9065); Min I = 2409742 + 143.6d*E R Sct |(JD2409730 - 12700); Min I = 2412755 + 141.5d*E R Sct |(JD2412750 - 16720); Min I = 2417161 + 139.5d*E R Sct |(JD2417150 - 20790); Min I = 2421083 + 143.4d*E R Sct |(JD2421050 - 25170) [09935]; Min I = 2429478 + 142.8d*E R Sct |(JD2429000 - 30650) [09938]; Min I = 2432078 + 140.05d*E R Sct |(JD2432000 - 42240) [07596]; Min I = 2442737 + 152.5d*E R Sct |(JD2442550 - 43050); Min I = 2443315 + 138.5d*E R Sct |(JD2443050 - 44150) [00001]; since JD2444150 - see Table. R Sct |Light curve drawings [09935,09936,9937]. R Sct |Spectrum description [09939,09954]. S Sct |VB A (B 11.9M V, 14.5", 238deg; C 12.5m V, 44", 105deg). U Sct |Min II 10.31. W Sct |Min II 10.1. X Sct |[A/H] = -0.1. In the region of the open cluster NGC 6639. Y Sct |In the region of the open cluster NGC 6664. Z Sct |[A/H] = 0.3. RS Sct |Min II 10.08. RU Sct |[A/H] = -0.7. P var. There is a nonlinear term in the RU Sct |elements given in the Table: +3.15d*10**(-6)*E**2. RX Sct |Connected with the bright hydrogen nebula YM 13. RY Sct |Min II 9.56. P var? Min I = 2427979.340 + 11.124939d*E RY Sct |(JD2414800 - 36100) [00007]; since JD2431200 - see Table. RY Sct |The shape of the light curve varies. RZ Sct |Min II 7.47. P var. There is nonlinear term in the RZ Sct |elements given in the Table: +0.78d*10**(-7)*E**2. SU Sct |P var. Max = 2424324.48 + 1.467713d*E (JD2420700 - 34310); SU Sct |Max = 2439678.428 + 1.468753d*E (JD2437100 - 41100) [07806]; SU Sct |since JD2441100 - see Table. TX Sct |CWA? red. TY Sct |[A/H] = -0.3. In the region of the open cluster Tr 35. UZ Sct |[Fe/H] = 0.35. P var. Max = 2435629.5 + 14.7468d*E UZ Sct |(JD2423900 - 35700) [02309]; since JD2436000 - see Table. VV Sct |SF component of a pair. VW Sct |P var. Max = 2415887 + 234d*E (JD2411900 - 22210); VW Sct |Max = 2423588 + 235d*E (JD2422880 - 27600); VW Sct |Max = 2429468 + 235.1d*E (JD2428750 - 34200); VW Sct |since JD2434600 - see Table. VX Sct |d = 0.064P. VZ Sct |Min II 12.0. WY Sct |P var. XY Sct |Min II 14.5. AC Sct |d = 0.024P; Min II 10.2. AE Sct |d = 0.04P. AI Sct |In the region of the open cluster NGC 6705. AN Sct |P var? AP Sct |V2 (NGC 6712). AU Sct |d ~0.03P. BC Sct |Following component of a close double system. The BC Sct |companion - NSV 11551. BH Sct |Min II 14.9. BI Sct |VB A (B 16.3m:, 3", 280deg; C 16.7m:, 12", 190deg; BI Sct |D 16.8m:, 18", 45deg; E 17.0m:, 6", 350deg). BK Sct |Close companion 16.5m sf. BN Sct |d = 0.02P. BP Sct |S 5.5/5.5. BS Sct |Min II 11.07. In the region of the open cluster M11 BS Sct |(NGC 6705). BU Sct |A var. P var. Max = 2425804.625 + 0.42022d*E [01401]; BU Sct |Max = 2427928.041 + 0.4202188d*E (JD2427900 - 9440) BU Sct |[01404]; Max = 2432770.464 + 0.4201944d*E BU Sct |(JD2432740 - 38290); Max = 2438589.357 + 0.4202171d*E BU Sct |(JD2438580 - 40510) [07806]; since JD2440770 - see Table. BX Sct |[A/H] = -0.9. CD Sct |Min II 13.7. CF Sct |d = 0.035P. CH Sct |V7 (NGC 6712). The member of this globular cluster. CK Sct |[Fe/H] = 0.23. CL Sct |May be the period should be doubled? CM Sct |[A/H] = 0.1. CN Sct |[A/H] = -1.5. CO Sct |P var? Resembles RV Tau type variables: if the period is CO Sct |doubled, the neight of max I and the depth of Min II vary. CR Sct |Min II 12.1; DII = 0.071P; Min II - Min I = 0.53P. CT Sct |Min II 11.1. CW Sct |Min II 10.1. CZ Sct |The epoch of Min brightness is given. DD Sct |One of the components probably varies. DE Sct |Min II 16.3. DG Sct |d = 0.03P:. DL Sct |Min II 15.9. DT Sct |Min II 16.5. DV Sct |Min II 17.8. DW Sct |Min II 16.4. EE Sct |Min II 15.3. EH Sct |Min II 15.0. EK Sct |Min II 16.0. EL Sct |The shape of the light curve varies? EN Sct |Min II 17.2. The different elements are also possible: EN Sct |Min I = 2428008.85 + 1.06446d*E. EP Sct |d = 0.04P:; Min II 15.6. EQ Sct |In the region of the open cluster NGC 6631. Min II 12.6:. ER Sct |Min II 9.3; Min II - Min I = 0.506P; DII = 0.14P. EU Sct |VB A (B 17.5m, 6", 45deg). EV Sct |[A/H] = -0.4. The member of the open cluster NGC 6664. EW Sct |P0 = 5.8195d (A/2 = 0.27m), P1 = 4.0646d (A/2 = 0.22m); EW Sct |P1/P0 = 0.6984. EX Sct |d = 0.025P:. EY Sct |Min II 12.4. In the region of the open cluster NGC 6683. EZ Sct |Min II 12.5. FF Sct |Min II 14.2. FG Sct |Min II 14.70. P var? Min I = 2429017.557 + 0.2705728d*E FG Sct |(JD2427975 - 29520) [01397]; since JD2444700 - see Table. FH Sct |In the region of the open cluster NGC 6694. FK Sct |Min II 14.4:. FL Sct |Min II 13.8. FM Sct |Min II 12.9. FN Sct |In the open cluster NGC 6704. FO Sct |D = 0.22d. FR Sct |Spectrum description [01410]. GI Sct |Min II 14.5. GM Sct |Min II 13.8:. HI Sct |D = 0.29d. HL Sct |Min II 13.4. IS Sct |P < 200d. IT Sct |In the region of the open cluster NGC 6705. LL Sct |sf component of a close pair. LR Sct |In the region of the globular cluster NGC 6712. LU Sct |P2 = 30d. LZ Sct |In the region of the globular cluster NGC 6712. MM Sct |Min II 15.8. MP Sct |V1 (NGC 6712). The member of this globular cluster. MP Sct |[Fe/H] = -0.69. MR Sct |V8 (NGC 6712). P var. Max = 2430885 + 117d*E MR Sct |(JD2427900 - 32400) [04231]; since JD2434900 - see Table. NU Sct |VB A (B 16.6m, 12", 180deg). NV Sct |P = 200d? OU Sct |P var. Max = 2427620 + 152d*E (JD2426200 - 32800); OU Sct |since JD2433100 - see Table. PT Sct |There is a close companion, 16.4m. PW Sct |The range of the combined light of the variable and PW Sct |a close companion, which follows, is given in the Table. QU Sct |The variable is also eclipsing one with P = 0.2d and QU Sct |A = 0.7m. V0337 Sct |A close companion (16.2m, <7", 90deg). V0340 Sct |Min II 15.6. V0356 Sct |Min II 12.3; DII = 0.10P. V0360 Sct |A close fn companion, 16.4m. V0362 Sct |P = 170d? V0367 Sct |In the open cluster NGC 6649. The light elements V0367 Sct |with fundamental mode period P0 (A0 = 0.54m B) are V0367 Sct |given in the Table. For the first-overtone period V0367 Sct |P1 (A1 = 0.41m B) Max = 2437435.12 + 4.38466d*E; V0367 Sct |P1/P0 = 0.696744. M - m var (0.15 <= M - m <= 0.45). V0369 Sct |In the region of the open cluster NGC 6705 (M 11). V0369 Sct |There is a superposition of the four light oscillations: V0369 Sct |P1 = 0.240d (A1 = 0.044m), P2 = 0.220d (A2 = 0.020m), V0369 Sct |P3 = 0.182d (A3 = 0.068m), P4 = 0.114d (A4 = 0.028m) V0369 Sct |[09745]. V0370 Sct |d = 0.016P. V0372 Sct |d = 0.012P. V0414 Sct |Blue companion? del Sct |VB A (B 10m, 53", 130deg); (k - b)2 = 0.37. del Sct |The basic light variation P0 (A0 = 0.125m) given in the del Sct |Table is superposed by the secondary one with del Sct |P1 = 0.1867756 (A1 = 0.034) [09975]. R Ser |P var. Max = 2372429 + 356.93d*E (JD2372400 - 88900) R Ser |[00960]; Max = 2397809 + 353.00d*E R Ser |(JD2394000 - 2403000); Max = 2403104 + 357.25d*E R Ser |(JD2403000 - 24000); Max = 2432387 + 356.10D*E R Ser |(JD2424000-39200); since JD2441000 - see Table. R Ser |Maser (SiO, H2O). S Ser |P var. Max = 2394360 + 361.01d*E (JD2394000 - 2407000); S Ser |Max = 2407024 + 372.70d*E (JD2407000 - 17000) [00960]; S Ser |Max = 2425875 + 366.59d*E (JD2417000 - 36000); since S Ser |JD2437600 - see Table. Maser (OH, SiO, H2O). T Ser |In the region of the open cluster NGC 6633. T Ser |P var. Max = 2400907 + 342.05d*E (JD2400500 - 15000); T Ser |Max = 2417912 + 345.73d*E (JD2417900 - 26000); T Ser |Max = 2428524 + 332.21d*E (JD2426000 - 32500); T Ser |Max = 2438382 + 345.71d*E (JD2432500 - 39500); since T Ser |JD2439500 - see Table. 0.8' from BN Ser. U Ser |P var. Max = 2421158 + 237.70d*E (JD2414000 - 22000); U Ser |Max = 2422347 + 236.78d*E (JD2422000 - 26600); U Ser |Max = 2426609 + 239.21d*E (JD2426600 - 32500); U Ser |since JD2432500 - see Table. V Ser |Min II 9.85. W Ser |P var, nonlinear terms: W Ser |+(3.140d*10**(-6))*E**2 + (1.432d*10**(-9))*E**3. W Ser |The light curve shape var. Wavelike variations in Max W Ser |light. Changes of emission lines with the orbital phase. W Ser |Active mass exchange, evidence for a common envelope. X Ser |After 1932 variations 14.3m - 18.3m were noted; according X Ser |to [01417], P = 275d. Observations in 1961 - 1964 did not X Ser |confirm P = 275d, fluctuations of light with a period of X Ser |several minutes were suspected [03625]. The spectral data X Ser |are for 1981. Y Ser |Epoch of min is given. According to [08643], variations Y Ser |with P ~400d are superimposed by P ~40d. Z Ser |The elements are valid during JD2422000 - 31000. RS Ser |Min II 11.4. RT Ser |Max (1920 - 1923). In the spectrum (1977 - 1979) there are RT Ser |emissions Halpha - Hdelta, HeI, HeII, [OI] etc. RT Ser |Absorptions TiO. RV Ser |Maser (H2O). VY Ser |[Fe/H] = -1.77, Delta(S) = 9. WW Ser |Maser (H2O). WX Ser |Maser (OH, SiO, H2O). P var? AA Ser |[A/H] = 0.2. AG Ser |P var? since JD2435000 - see Table. AK Ser |P var? before JD2442300 Min = 2431313.266 + 1.9225667d*E AK Ser |[00318]; since JD2442300 - see Table. AN Ser |P var? Max = 2429156.260 + 0.5220703d*E AN Ser |(JD2427000 - 38000) [00001]; since JD2438000 - see Table. AN Ser |According to [02740], Blazhko effect with Pi = 21.94d; AN Ser |the presence of the Blazhko effect is denied in [07258]. AN Ser |Delta(S) = 0. AO Ser |Min II 10.8. AP Ser |VB A (B 14.29m, 8" sp). [Fe/H] = -1.37. AQ Ser |Min II 11.1. AR Ser |P var. Before JD2425000 Max = 2415617.698 + 0.5752221d*E; AR Ser |Max = 2425313.530 + 0.57508945d*E AR Ser |(JD2425000 - 28500); Max = 2428848.662 + 0.575214d*E AR Ser |(JD2428500 - 31000) [08081]; Max = AR Ser |2431436.424 + 0.5751134d*E (JD2431000 - 34200); AR Ser |Max = 2436013.279 + 0.5752169d*E (JD2435900 - 37200); AR Ser |Max = 2438138.467 + 0.5750651d*E (JD2437200 - 38700) AR Ser |[00001]. Elements working on average since JD2438700 - see AR Ser |Table. Complex Blazhko effect. Pi = 108.4d [08082]. AR Ser |A var (0.23m - 0.87m V). Pi var (80d - 120d) [07032]. AR Ser |Delta(S) = 4.6. AS Ser |Min II 11.5. The epoch of Min I 2442937.428 AS Ser |(BBSAG) is not in agreement with the elements. AT Ser |P var. Max = 2415353.783 + 0.74655695d*E AT Ser |(JD2415000 - 27000); Max = 2428337.260 + 0.7465670d*E AT Ser |(JD2428000 - 39500); since JD2441500 - see Table. AT Ser |Delta(S) = 9. AU Ser |Min II 11.61. AU Ser |The light curve shape var. AV Ser |Delta(S) = 6. AW Ser |Delta(S) = 5.0. BF Ser |[A/H] = -2.5. Delta(S) = 6. BH Ser |P var. Max = 2427956.674 + 0.434545d*E (JD2425000 - BH Ser |30700) [01039]; since JD2437650 - see Table. BI Ser |Min I 2446264.414 [10200] contradicts the elements. P var? BN Ser |In the region of the open cluster NGC 6633. 0.8' from BN Ser |T Ser. BO Ser |P var? Max = 2425681 + 201d (JD2425600 - 30100) 0447]; BO Ser |the Table gives mean elements (JD2425600 - 35400). BQ Ser |P0 - see Table. P1 = 3.012d [08188]. In the region of the BQ Ser |open cluster IC 4756. BR Ser |In the region of the open cluster IC 4756. BS Ser |In the region of the open cluster IC 4756. BT Ser |In the region of the open cluster IC 4756. BU Ser |In the region of the open cluster IC 4756. CC Ser |Min II 11.63. CN Ser |[Fe/H] = -0.77. Delta(S) = 3.4. CO Ser |P var? The light curve shape var. CO Ser |[Fe/H] = -1.38. Delta(S) = 7.2. CQ Ser |Min II 12.0. CR Ser |[A/H] = -0.2. CS Ser |P var. Max = 2418137.875 + 0.5267904d*E CS Ser |(JD2416000 - 32500) [00001]; since JD2432500 - see Table. CS Ser |Delta(S) = (6). In the region of the HII complex S 54 and CS Ser |the open star cluster NGC 6604. Connected with a CS Ser |shell-structure nebula. Sometimes eclipses are observed CS Ser |during the configuration "WR in front of O" (see Table) CS Ser |and sometimes during the configuration "O in front of CS Ser |WR" which coincided with the deepest eclipse ever observed CS Ser |(with the depth 0.5m B, V). Sometimes the photometric CS Ser |eclipse at predicted moments does not occur, and only the CS Ser |atmospheric eclipse of the O star with the WR component is CS Ser |observed at lambda 4653 A (emission of CII - CIV, NIII), CS Ser |lambda < 2000 A. IR excess; possibly an IR eclipse in CS Ser |the configuration "O in front of WR". CX Ser |The light curve (resembling the eclipsing light curve of CX Ser |U Gem) shows a hump of ~0.2m height before the minimum; CX Ser |fluctuations up to ~0.3m - 0.4m in Max. DF Ser |VB A (B 13.9m, 0.4', -115deg). DG Ser |Min II 16.5:. The alias period is possible (0.3360742d). DH Ser |Another possible P = 450d. DK Ser |Max 2433829 [10008] contradicts the elements. DR Ser |VB A (B 12.54m, 28", 0deg). DT Ser |VB A (B ~5"). The spectrum shows emissions of [OIII] DT Ser |lambda lambda 4959, 5007 A. Symbiotic? [08676]. DV Ser |In a small star cluster. DY Ser |[Fe/H] = -1.58. Delta(S) = 8.4. EE Ser |In the region of the open cluster M 17 = NGC 6618. EF Ser |In the region of the open cluster M 17 = NGC 6618. EG Ser |VB A (ro > 10"). EL Ser |N <= 7. EN Ser |[Fe/H] = -1.07. Delta(S) = 5.3. EO Ser |The light curve shows large scatter. RR(B) type is EO Ser |possible. Max = 2437433.653 + 0.6309d*E (JD2437433 - 514) EO Ser |[3625]. [Fe/H] = -1.63. Delta(S) = 8.8. ER Ser |In the region of the open cluster M 16 = NGC 6611. ES Ser |In the region of the open cluster M 16 = NGC 6611. ET Ser |In the region of the open cluster M 16 = NGC 6611. EU Ser |VB A (B 4" np). A member of the open cluster EU Ser |M 16 = NGC 6611. IR excess. EV Ser |In the region of the open cluster M 16 = NGC 6611. EW Ser |In the region of the open cluster M 16 = NGC 6611. EX Ser |In the region of the open cluster M 16 = NGC 6611. FI Ser |Hints of periodicity in U light. FK Ser |VB (Delta(m) ~0.5m, 1.3", 11.5deg, 1972). FK Ser |Flares were found in the satellite UV range [10013]. FK Ser |Differences from typical by stars and probable "post-T Tau" FK Ser |nature are noted [07260,03866]. According to [06948], FK Ser |Min = 2441939.200 + 5.20d*E. Soft X-ray source. FL Ser |VB (Delta(m) = 1.9m, 0.46", 145deg, 1981). FM Ser |In the region of the open cluster M 16 = NGC 6611. FM Ser |VB (var sf?). FN Ser |In the region of the open cluster M 16 = NGC 6611. FR Ser |ADS 11477 A (B 12.5m, 10.5", 330deg, 1924; C 9.3m, FR Ser |30.5", 5deg, 1930). Possible values of P: 2.1308d, 2.1565d. LN Ser |m pg ~17.5m ~const; blue companion? [07264]. LS Ser |The light curve shows large scatter, the elements need LS Ser |confirmation. Possible identification with an X-ray source LS Ser |2ASE 1822 + 0. LV Ser |The epoch of max in V light is given; in B and U varies LV Ser |in opposite phase. LX Ser |The depth of eclipses ~2.5m. Comparatively frequent LX Ser |outbursts [10023]. MM Ser |Ser X-1 = 4 U 1 837 + 04. LX/Lopt >= 100. MM Ser |VB B (A 19.1m; B 2.2", 210deg). MO Ser |V1 (NGC 6535). Cluster non-member. MP Ser |V2 (NGC 6535). Cluster non-member. OU Ser |SB2. PS Ser |Both components are SB systems, Porb(A) = 15.888d, PS Ser |Porb(B) = 13.561d. PT Ser |SB, Porb = 38.937d. del Ser |ADS 9701A (B 5.16m, dF0, a = 5.843", Porb = 3168 yr; del Ser |4", 175G, 1980). omi Ser |SB? d Ser |ADS 11353 A (B 7.44m, SB?, F5V, 3.9", 320deg, 1983). d Ser |VB (speckle-interferometric; 0.25", 157deg, 1976). d Ser |SB (P1orb = 385d, P2orb = 1.8505205d). S Sex |P var. Max = 2422029 + 257.2d*E (JD2417650 - 22050); S Sex |Max = 2428968 + 266.65d*E (JD2422050 - 30300); Max = S Sex |2434739 + 260.86d*E (JD2430300 - 34750); Max = S Sex |2438796 + 254.3d*E (JD2434750 - 38800); S Sex |since JD2440600 - see Table. T Sex |[Fe/H] = -1.20. P var. Max = 2416146.675 + 0.32465971d*E T Sex |(JD2414000 - 18300), Max = 2424561.398 + 0.32467107d*E T Sex |(JD2418300 - 24570) [00752]; T Sex |Max = 2424561.430 + 0.3246702d*E (JD2424560 - 28280), T Sex |Max = 2429350.320 + 0.3247113d*E (JD2429350 - 34370), T Sex |Max = 2434795.409 + 0.3246978d*E (JD2434795 - 36630) T Sex |[09978]; since JD2441380 - see Table. U Sex |P var. Max = 2419823.355 + 0.53402622d*E U Sex |(JD2419470 - 36670) [03697]; since JD2443980 - see Table. Y Sex |Min II 10.17; dII = 0.05P. P var. Min I = 2428122.700 + Y Sex |0.41982341d*E (JD < 2429000) [00007]; Min I = Y Sex |2434445.989 + 0.419818d*E (JD2428100 - 35000) Y Sex |[00001], Min I = 2439521.964 + 0.41981543d*E Y Sex |(JD2431150 - 43250) [09981]; since JD2440300 - see Table. RU Sex |Min II 11.4. According to [09923], RR? RU Sex |(P = 0.5398d?), CEP? (P = 6.792d?). RW Sex |Porb = 0.247d [09925]; LX/Lopt = 10**(-4) [09926]; RW Sex |Px = 254s [09927]. RX Sex |VB A (B 9.1m, 116.3", 191deg). RY Sex |Mu = 0.67", P = 281deg. R Tau |OH, H2O, Sio maser. P var. Max = 2411012 + R Tau |325.0d*E (JD2398654 - 2414000); Max = 2424243 + R Tau |322.1d*E (JD2414000 - 24300); Max = 2434005 + R Tau |325.4d*E (JD2424300 - 35500); since JD2435500 - see Table. S Tau |P var. Max = 2404646 + 380.1d*E (JD2399326 - 2405000); S Tau |Max = 2425085 + 371.40d*E (JD2405000 - 26000); since S Tau |JD2426000 - see Table. T Tau |VB A (B 15m, 0.27", 358deg; C - infrared companion, 0.590", T Tau |180deg). Near the variable nebula NGC 1555. OH, H2O maser. T Tau |In the interval JD2402140 - 21000 the light range T Tau |9.3m - 13.5m, since JD2421000 - only 9.5m - 10.8m. U Tau |VB (A 10.9m; B 12.0m, 3", 77deg). V Tau |P var. Max = 2417978 + 170.0d*E (JD2404550 - 18000); V Tau |Max = 2424580 + 169.3d*E (JD2418000 - 24600); V Tau |Max = 2432746 + 170.1d*E (JD2424600 - 33500); V Tau |Max = 2436970 + 168.7d*E (JD2433500 - 37300); V Tau |Max = 2442442 + 171.1d*E (JD2437300 - 43000); V Tau |since JD2443000 - see Table. W Tau |<P> value is given in the Table. W Tau |P var. Max = 2415320 + 274.1d*E (JD2410360 - 15500), W Tau |Max = 2421995 + 266.1d*E (JD2415500 - 22500), W Tau |Max = 2425135 + 260.5d*E (JD2422500 - 28800), W Tau |Max = 2438837 + 245.4d*E (JD2428800 - 39100) [00001]. Z Tau |VB A (B 13.6m, 4", 45deg). Z Tau |P var. Max = 2425115 + 499.90d*E (JD2415100 - 26500) Z Tau |Max = 2438768 + 486.20d*E (JD2426500 - 39000); Z Tau |since JD2439000 - see Table. RR Tau |Spectrum description and the photographs of the nebula RR Tau |[04002]. RU Tau |VB A (B 4"). P var. Max = 2426004 + 545.3d*E RU Tau |(JD2415009 - 27500). Max = 2434309 + 604.0d*E RU Tau |(JD2427500 - 34500); since JD2437500 - see Table. RV Tau |OH maser. Mean brightness varies: Min = 2417553 + 1224d*E RV Tau |[00580]. RW Tau |VB A (12.5m, 1.3", 172deg, 1959). dI = 0.020P; Min II 8.09. RW Tau |P var. Min I = 2417198.410 + 2.7688665d*E + RW Tau |0.038d*sin(0.0818deg*(E - 100)) (JD2409913 - 24150), RW Tau |Min I = 2434423.3571 + 2.7688209d*E (JD2424150 - 37000) RW Tau |[05460]; Min I = 2437164.4860 + 2.7688480d*E RW Tau |(JD2437000 - 39900) [07531]; Min I = 2442776.93772 + RW Tau |2.76884463d*E (JD2439855 - 42780) [08593]; Min I = RW Tau |2442776.9313 + 2.7688396d*E (JD2442780 - 45750) RW Tau |[09084]; since JD2445750 - see Table. The shape of the RW Tau |light curve varies. RX Tau |OH, H2O maser. P var. Max = 2423561 + 338.4d*E RX Tau |(JD2417155 - 24000); Max = 2430505 + 330.2d*E RX Tau |(JD2424000 - 30700); Max = 2437963 + 339.3d*E RX Tau |(JD2430700 - 38000); since JD2438000 - see Table. RY Tau |SB1. The photographs of the nebula and spectrum RY Tau |description [05064]. Long period light variations are RY Tau |possible with cycles 70.25, 15.9, 9.4 and 5.84 years RY Tau |[09993]. RZ Tau |Min II 10.66. P var. Min I = 2424032.1426 + RZ Tau |0.41567109d*E (JD2424000 - 34100) [00312]; RZ Tau |since JD2436000 - see Table. SS Tau |P var [03506]. Max = 2420894.2339 + 0.3699665d*E SS Tau |(JD2420890 - 21300) [09995]; Max = 2426669.080 + SS Tau |0.3699687d*E (JD2426400 - 26700) [00320]; Max = SS Tau |2428843.856 + 0.3699231d*E (JD2426700 - 30300), SS Tau |Max = 2431392.603 + 0.369912d*E (JD2430300 - 31400), SS Tau |Max = 2432118.794 + 0.369937d*E (JD2431400 - 32150), SS Tau |Max = 2432857.884 + 0.3699146d*E (JD2432150 - 35000), SS Tau |Max = 2435055.528 + 0.3699066d*E (JD2435000 - 36400), SS Tau |Max = 2437313.503 + 0.3699266d*E (JD2436400 - 37320), SS Tau |Max = 2437960.419 + 0.369878d*E (JD2437300 - 37960), SS Tau |Max = 2437960.419 + 0.369938d*E (JD2437960 - 38740); SS Tau |since JD2438740 - see Table. SV Tau |Min II 9.8. SW Tau |P var. Max = 2432049.856 + 1.583623d*E (JD2418240 - 36000); SW Tau |since JD2436000 - see Table. SX Tau |In the region of the Pleiades cluster. Not a member SX Tau |of the cluster. SY Tau |In the region of the Pleiades cluster. Not a member SY Tau |of the cluster. SZ Tau |The member of the halo of the open cluster NGC 1647. SZ Tau |P var. Max = 2410000.60 + 3.1487d*E (JD2412000 - 20200) SZ Tau |[09996]; Max = 2419267.519 + 3.149046d*E SZ Tau |(JD2419260 - 34650); since JD2434650 - see Table. TT Tau |P = 364d? [00589]. TY Tau |In the region of the hyades cluster. Not a member of TY Tau |the cluster. According to [09997], Min = 2422291.303 + TY Tau |0.539250d*E. UU Tau |In the region of the Pleiades cluster. Not a member of UU Tau |the cluster. UX Tau |VB A (B 13.67m V, M2.5 VE, 5.74", 270.1deg, 1944). UZ Tau |VB A (B 15.16m B, M4VE (Li), 3.7", 271.5deg, 1944). UZ Tau |The range of the combined light variation is given in the UZ Tau |Table. VW Tau |The chart in [06286] is wrong. WW Tau |P var. P = 114.8d (JD2414800 - 20800). P = 124.4d WW Tau |(JD2420800 - 23700) [00634]; P = 114d (JD2424800 - 26300), WW Tau |P = 139d (JD2426300 - 27700) [00310]; P = 114d WW Tau |(JD2427900 - 30800), P = 131d (JD2430800 - 31500), WW Tau |P = 109d (JD2431500 - 33400) [00364]; since WW Tau |JD2433400 - see Table. WY Tau |Min II 11.73. P var? [10048]. WZ Tau |VB. XZ Tau |VB A (B = HL Tau, 23", 273deg). YZ Tau |[Fe/H] = -1.53. In the region of the Pleiades cluster. YZ Tau |Not a member of the cluster. YZ Tau |There is a square term in the elements: -6d*10**(-11)*E**2. AA Tau |Cyclic light variation with P = 4.5d and 2d [10003] and AA Tau |also 8.2d [10004] is possible. AC Tau |d = 0.025P. P var? AH Tau |Min II 11.85. P var? In the region of the Pleiades AH Tau |cluster. Not a member of the cluster. AL Tau |P var. The depth of Min II 0.15m. AM Tau |d = 0.012P:. P var. Min I = 2427534.444 + 2.044018d*E AM Tau |(JD2425580 - 27540), Min I = 2435019.436 + AM Tau |2.043935d*E (JD2433320 - 37020); since JD2442365 - see AM Tau |Table. AN Tau |Min II 10.5; Min II - Min I = 0.53P. P var. AP Tau |Min II 14.7; Min II - Min I = 0.48P. AS Tau |P var. Min I = 2439390.595 + 3.4835542d*E AS Tau |(JD2419440 - 44300) [07806]; since JD2444300 - see Table. AU Tau |P var. Max = 2426642 + 71.0d*E (JD2426290 - 30400) AU Tau |[00310]; since JD2438000 - see Table. AW Tau |OH, H2O maser. P var. Max = 2426278 + 690d*E AW Tau |(JD2416100 - 33850) [00609]; since JD2433850 - see Table. BB Tau |SC 7/7 e. BK Tau |In the region of the Pleiades cluster. Not a member of BK Tau |the cluster. BN Tau |P var. Min I = 2435460.370 + 4.2542044d*E BN Tau |(JD2419000-39100) [05466]; since JD2443000 - see Table. BP Tau |There are quasisinusoidal light variations with P = 7.6d BP Tau |[10011]. BU Tau |Pleione. The member of the Pleiades cluster. BV Tau |Min II 11.9. BW Tau |3C 120. Seyfert galaxy; Z = 0.033. Spectrum description BW Tau |[10012]. CD Tau |VB A (B 9.88m, 9.9", 148.8deg). Min II 7.31. CD Tau |In the region of the open cluster CR 65. CF Tau |d = 0.02P; Min II 10.2; CH Tau |The epoch of Min brightness is given. CM Tau |SN 1054 in the Crab nebula (NGC 1952 = M1); pulsar NP 0532. CM Tau |The outburst epoch is JD2106210:. The pulsed radiation CM Tau |varies precisely in phase over the whole spectrum, from CM Tau |radio waves to gamma rays with P = 0.033S in the range CM Tau |13.9m - 17.7m V. P var [10017,10018]: 0.033095563927s CM Tau |(JD2440297.5094) <= P <= 0.033242051159s (JD2444312.750). CR Tau |P = 1.362692d? CT Tau |Min II 11.12. P var. Min I = 2437312.369 + 0.6668274d*E CT Tau |(JD2432700 - 38790) [10010]; since JD2441400 - see Table. CU Tau |In the region of the Pleiades cluster. Not a member of CU Tau |the cluster. Min II 11.90. P var. Min I = CU Tau |2431822.5193 + 0.4126022d*E (JD2431060 - 2890) CU Tau |[00604]; since JD2440960 - see Table. CZ Tau |VB B (A = DD Tau; B 31", 13deg). DD Tau |VB A (B = CZ Tau; 31", 13deg. DE Tau |VB A (B 26", 10deg). DG Tau |Connected with a small bright arc-shaped nebula. DH Tau |VB A (B = DI Tau, 16", 125deg). According to [10004] there DH Tau |is periodical light variability with P = 7.0d and DH Tau |A = 0.4m V. DI Tau |VB B (A = DH Tau; B 16", 125deg). DI Tau |According to [10004] there is DI Tau |periodical light variability with P ~7.0d and A < 0.4m V. DL Tau |VB A (B 17m V, 12", 333deg). DL Tau |Cyclic light variation with P = 2.7d is present [10003]. DN Tau |There are sinusoidal light variations with DN Tau |P = 6.6d [10011]. DO Tau |Connected with a small bright arc-shaped nebula. DS Tau |VB A (B 13.7m, 4", 288deg). Range of Combined light DS Tau |variation of the pair is given in the Table. EI Tau |VB? EQ Tau |Min II 10.97. In the region of the Pleiades cluster. EQ Tau |Not a member of the cluster. ES Tau |Min II 14.4; Min II - Min I = 0.52P; d = 0.005P. ET Tau |Min II 9.3. EY Tau |The member of the Hyades cluster. EZ Tau |The member of the Hyades cluster. FH Tau |The member of the Hyades cluster. FL Tau |The member of the Pleiades cluster. FS Tau |VB A (B 16", 289deg). FV Tau |VB A (B 13", 103deg). FW Tau |VB A (B 13", 243deg). FY Tau |VB B (A = FZ Tau, B 17", 250deg.) FZ Tau |VB A (B = FY Tau, 17", 250deg). GG Tau |VB A (B 18.5m, 12", 205deg). GH Tau |VB B (A = V807 Tau; B 21.4", 193deg). GI Tau |VB B (A = GK Tau; B 13", 329deg). There are GI Tau |quasisinusoidal light variations with P = 7.2d [10011]. GI Tau |Connected with a small bright arc-shaped nebula. GK Tau |VB A (B = GI Tau, 13", 329deg). GK Tau |There are quasisinusoidal light variations with P = 4.6d GK Tau |[10011]. Connected with a small bright arc-shaped nebula. GL Tau |The central star of the planetary nebula PK 174 -14deg 1. GP Tau |P2 = 1000d. GR Tau |dI = 0.068P; Min II 10.49; Mim II - Min I = 0.516P. GS Tau |SB1 (Porb = 7.227424d [06568]). The epoch of Min GS Tau |brightness is given. GU Tau |VB A (B 11", 299deg). GV Tau |Herbig-haro object. GW Tau |Min II 11.7. P var? GX Tau |VB A (B 11", 310deg). HK Tau |VB A (B 21m, 2", 180deg). HL Tau |VB B (A = XZ Tau; B 23", 273deg). Connected with a HL Tau |small bright arc-shaped nebula. HN Tau |VB A (B 18m, 3.3", 205deg). HO Tau |VB A (B 8", 110deg). HP Tau |Connected with a small bright arc-shaped nebula. HP Tau |According to [10004] there is periodical variability HP Tau |with P = 1.2d. HR Tau |VB B (A = HS Tau; B 14", 119deg). HS Tau |VB A (B = HR Tau; 14", 119deg). HU Tau |Min II 5.91. HW Tau |Minor planet (49) Pales. HZ Tau |In the region of the Pleiades cluster. Possible HZ Tau |member of the cluster. II Tau |In the region of the Pleiades cluster. II Tau |Possible member of the hyades cluster IK Tau |OH, H2O, SiO maser. IM Tau |P var. Max = 2439792.398 + 0.144969d*E (JD2439790 - IM Tau |43130) [10019]; P1 = 0.109016d, P1/P0 = 0.752. IM Tau |Since JD2444230 - see Table. IN Tau |mu = 0.121", P = 105deg. The member of the Hyades cluster? IO Tau |In the region of the Hyades cluster. IQ Tau |VB A (B 17m, 11", 298deg). IS Tau |SVS 1319 [04051]. IS Tau |The star N23 with Halpha emission [00596]. In the map given IS Tau |in [00596] erroneously designated as N26 in contradiction IS Tau |with the co-ordinates given in the same paper. It was the IS Tau |reason for different mistakes when the IS Tau |star was identified by some other investigators. IT Tau |SVS 1320 [04051]. IT Tau |The star N26 with Halpha emission [00596]. IT Tau |In the map given in [00596] IS Tau erroneously designated IT Tau |as N26 in contradiction with the co-ordinates given in the IT Tau |same paper. It was the reason for different mistakes when IT Tau |IS Tau was identified by some other investigators. KK Tau |In the region of the Pleiades cluster. KL Tau |In the region of the Pleiades cluster. KM Tau |In the region of the Pleiades cluster. KN Tau |In the region of the Pleiades cluster. KO Tau |In the region of the Pleiades cluster. KP Tau |In the region of the Pleiades cluster. Not a member KP Tau |of the cluster. KQ Tau |In the region of the Pleiades cluster. KR Tau |In the region of the Pleiades cluster. Not a member KR Tau |of the cluster. KS Tau |In the region of the Pleiades cluster. KT Tau |In the region of the Pleiades cluster. KU Tau |In the region of the Pleiades cluster. KV Tau |In the region of the Pleiades cluster. KW Tau |In the region of the Pleiades cluster. KX Tau |In the region of the Pleiades cluster. Not a member KX Tau |of the cluster. KY Tau |The member of the Pleiades cluster. KZ Tau |In the region of the Pleiades cluster. LL Tau |In the region of the Pleiades cluster. LM Tau |In the region of the Pleiades cluster. Possible member LM Tau |of the cluster. LN Tau |In the region of the Pleiades cluster. LO Tau |In the region of the Pleiades cluster. Possible member LO Tau |of the cluster. LP Tau |In the region of the Pleiades cluster. Not a member LP Tau |of the cluster. LQ Tau |In the region of the Pleiades cluster. LR Tau |In the region of the Pleiades cluster. Possible member LR Tau |of the Hyades cluster. LS Tau |In the region of the Pleiades cluster. LT Tau |In the region of the Pleiades cluster. Possible member LT Tau |of the cluster. LU Tau |In the region of the Pleiades cluster. Possible member LU Tau |of the cluster. LV Tau |In the region of the Pleiades cluster. Possible member LV Tau |of the cluster. LW Tau |In the region of the Pleiades cluster. Not a member LW Tau |of the cluster. LX Tau |In the region of the Pleiades cluster. LY Tau |In the region of the Pleiades cluster. Possible member LY Tau |of the cluster. LZ Tau |The member of the Pleiades cluster. MM Tau |The member of the Pleiades cluster. MN Tau |In the region of the Pleiades cluster. MO Tau |In the region of the Pleiades cluster. Possible member MO Tau |of the cluster. MP Tau |In the region of the Pleiades cluster. MQ Tau |In the region of the Pleiades cluster. MR Tau |The member of the Pleiades cluster. MS Tau |The member of the Pleiades cluster. MT Tau |In the region of the Pleiades cluster. Not a member MT Tau |of the cluster. MU Tau |In the region of the Pleiades cluster. Possible member MU Tau |of the cluster. MV Tau |In the region of the Pleiades cluster. Possible member MV Tau |of the cluster. MW Tau |In the region of the Pleiades cluster. MX Tau |The member of the Pleiades cluster. MY Tau |The member of the Pleiades cluster. MZ Tau |In the region of the Pleiades cluster. Possible member MZ Tau |of the cluster. NN Tau |In the region of the Pleiades cluster. NO Tau |In the region of the Pleiades cluster. NP Tau |The member of the Pleiades cluster. NQ Tau |In the region of the Pleiades cluster. NR Tau |In the region of the Pleiades cluster. Not a member NR Tau |of the cluster. NS Tau |In the region of the Pleiades cluster. NT Tau |In the region of the Pleiades cluster. Possible member NT Tau |of the cluster. NU Tau |In the region of the Pleiades cluster. NV Tau |In the region of the Pleiades cluster. Not a member NV Tau |of the cluster. NW Tau |In the region of the Pleiades cluster. NX Tau |In the region of the Pleiades cluster. Not a member NX Tau |of the cluster. NY Tau |In the region of the Pleiades cluster. Not a member NY Tau |of the cluster. NZ Tau |In the region of the Pleiades cluster. OO Tau |In the region of the Pleiades cluster. OP Tau |In the region of the Pleiades cluster. Possible member OP Tau |of the cluster. OQ Tau |In the region of the Pleiades cluster. OR Tau |The member of the Pleiades cluster. OS Tau |The member of the Pleiades cluster. OT Tau |The member of the Pleiades cluster. OU Tau |Max = 2444896.758 + 0.39701d*E, M - m = 0.5P, A(V) = OU Tau |0.13m [10052]. OU Tau |The member of the Pleiades cluster. OW Tau |The member of the Pleiades cluster. OX Tau |In the region of the Pleiades cluster. OY Tau |In the region of the Pleiades cluster. Not a member OY Tau |of the cluster. OZ Tau |In the region of the Pleiades cluster. Possible member OZ Tau |of the cluster. PP Tau |In the region of the Pleiades cluster. Possible member PP Tau |of the cluster. PQ Tau |In the region of the Pleiades cluster. Not a member PQ Tau |of the cluster. PR Tau |The member of the Pleiades cluster. PS Tau |In the region of the Pleiades cluster. PT Tau |The member of the Pleiades cluster. PU Tau |In the region of the Pleiades cluster. PV Tau |In the region of the Pleiades cluster. Possible member PV Tau |of the cluster. PW Tau |In the region of the Pleiades cluster. PZ Tau |In the region of the Pleiades cluster. QQ Tau |SB2. The member of the Pleiades cluster. QR Tau |In the region of the Pleiades cluster. QS Tau |In the region of the Pleiades cluster. QT Tau |In the region of the Pleiades cluster. QU Tau |VB A (B 18.0m, 4.0", 135deg). In the region of the QU Tau |Pleiades cluster. QV Tau |In the region of the Pleiades cluster. QW Tau |In the region of the Pleiades cluster. QX Tau |The member of the Pleiades cluster. QX Tau |Max = 2444896.79 + 0.483d*E, M - m = 0.5P, A(V) = 0.125m QX Tau |[10052]. QY Tau |In the region of the Pleiades cluster. Not a member QY Tau |of the cluster. QZ Tau |In the region of the Pleiades cluster. V0335 Tau |In the region of the Pleiades cluster. V0336 Tau |In the region of the Pleiades cluster. Possible member V0336 Tau |of the cluster. V0337 Tau |In the region of the Pleiades cluster. V0338 Tau |In the region of the Pleiades cluster. Possible member V0338 Tau |of the cluster. V0339 Tau |In the region of the Pleiades cluster. Not a member V0339 Tau |of the cluster. V0340 Tau |In the region of the Pleiades cluster. V0341 Tau |In the region of the Pleiades cluster. V0342 Tau |In the region of the Pleiades cluster. V0343 Tau |The member of the Pleiades cluster. V0344 Tau |In the region of the Pleiades cluster. V0345 Tau |In the region of the Pleiades cluster. V0346 Tau |The member of the Pleiades cluster. V0347 Tau |In the region of the Pleiades cluster. Not a member V0347 Tau |of the cluster. V0348 Tau |In the region of the Pleiades cluster. V0349 Tau |In the region of the Pleiades cluster. Possible member V0349 Tau |of the cluster. V0350 Tau |In the region of the Pleiades cluster. Possible member V0350 Tau |of the cluster. V0351 Tau |In the region of the Pleiades cluster. Not a member V0351 Tau |of the cluster. V0352 Tau |In the region of the Pleiades cluster. V0353 Tau |In the region of the Pleiades cluster. Possible member V0353 Tau |of the cluster. V0354 Tau |In the region of the Pleiades cluster. Possible member V0354 Tau |of the cluster. V0355 Tau |In the region of the Pleiades cluster. Possible member V0355 Tau |of the cluster. V0356 Tau |In the region of the Pleiades cluster. V0357 Tau |The member of the Pleiades cluster. V0358 Tau |The member of the Pleiades cluster. V0359 Tau |In the region of the Pleiades cluster. V0360 Tau |In the region of the Pleiades cluster. V0361 Tau |In the region of the Pleiades cluster. Possible member V0361 Tau |of the cluster. V0362 Tau |In the region of the Pleiades cluster. V0363 Tau |In the region of the Pleiades cluster. Possible member V0364 Tau |In the region of the Pleiades cluster. Possible member V0364 Tau |of the cluster. V0365 Tau |In the region of the Pleiades cluster. V0366 Tau |The member of the Pleiades cluster. V0367 Tau |In the region of the Pleiades cluster. V0368 Tau |In the region of the Pleiades cluster. V0369 Tau |In the region of the Pleiades cluster. V0370 Tau |The member of the Pleiades cluster. V0371 Tau |VB (Delta(m) ~1m, 1.5"). The member of the Pleiades V0371 Tau |cluster. V0372 Tau |The member of the Pleiades cluster. V0373 Tau |In the region of the Pleiades cluster. V0374 Tau |In the region of the Pleiades cluster. V0375 Tau |In the region of the Pleiades cluster. Not a member V0375 Tau |of the cluster. V0376 Tau |The member of the Pleiades cluster. V0377 Tau |The member of the Pleiades cluster. V0378 Tau |The member of the Pleiades cluster. V0379 Tau |In the region of the Pleiades cluster. Possible member V0379 Tau |of the cluster. V0380 Tau |In the region of the Pleiades cluster. Possible member V0380 Tau |of the cluster. V0381 Tau |The member of the Pleiades cluster. V0382 Tau |The member of the Pleiades cluster. V0383 Tau |In the region of the Pleiades cluster. V0384 Tau |The member of the Pleiades cluster. V0385 Tau |In the region of the Pleiades cluster. Not a member V0385 Tau |of the cluster. V0386 Tau |TCSN 437. In the region of the Pleiades cluster. V0387 Tau |In the region of the Pleiades cluster. V0388 Tau |In the region of the Pleiades cluster. V0389 Tau |TCSN 439. In the region of the Pleiades cluster. V0390 Tau |In the region of the Pleiades cluster. V0392 Tau |In the region of the Pleiades cluster. Possible member V0392 Tau |of the cluster. V0394 Tau |In the region of the Pleiades cluster. Not a member V0394 Tau |of the cluster. V0395 Tau |In the region of the Pleiades cluster. V0396 Tau |In the region of the Pleiades cluster. V0397 Tau |In the region of the Pleiades cluster. V0398 Tau |In the region of the Pleiades cluster. Possible member V0398 Tau |of the cluster. V0399 Tau |The member of the Pleiades cluster. V0400 Tau |In the region of the Pleiades cluster. V0401 Tau |In the region of the Pleiades cluster. V0402 Tau |The member of the Pleiades cluster. V0403 Tau |The member of the Pleiades cluster. V0404 Tau |In the region of the Pleiades cluster. V0405 Tau |In the region of the Pleiades cluster. V0410 Tau |There are periodical light variations with P = 1.92d, V0410 Tau |A(V) = 0.21m, M - m = 0.5P [10056]. V0411 Tau |mu = 0.13", P = 143deg. V0411 Tau |Eruptive white dwarf. Usually there are quasi-perio- V0411 Tau |dic variations with A ~0.3m and periods P0 = 12.436 V0411 Tau |Min and P1 = 8.237 Min (P1/P0 = 0.6624) which are V0411 Tau |nonlinearly modulated by the third period PL ~0.135d V0411 Tau |(probably by the orbital period of a faint companion). V0421 Tau |Minor planet (586) Thekla. V0423 Tau |Min II 15.8. V0425 Tau |In the region of the Pleiades cluster. Not a member V0425 Tau |of the cluster. V0426 Tau |In the region of the Pleiades cluster. V0427 Tau |In the region of the Pleiades cluster. V0428 Tau |In the region of the Pleiades cluster. V0429 Tau |In the region of the Pleiades cluster. V0430 Tau |In the region of the Pleiades cluster. Possible member V0430 Tau |of the cluster. V0431 Tau |In the region of the Pleiades cluster. V0432 Tau |In the region of the Pleiades cluster. V0433 Tau |In the region of the Pleiades cluster. V0434 Tau |In the region of the Pleiades cluster. V0435 Tau |In the region of the Pleiades cluster. Possible member V0435 Tau |of the cluster. V0436 Tau |In the region of the Pleiades cluster. Not a member V0436 Tau |of the cluster. V0437 Tau |In the region of the Pleiades cluster. Not a member V0437 Tau |of the cluster. V0438 Tau |In the region of the Pleiades cluster. Possible member V0438 Tau |of the cluster. V0439 Tau |In the region of the Pleiades cluster. V0440 Tau |In the region of the Pleiades cluster. V0441 Tau |In the region of the Pleiades cluster. Possible member V0441 Tau |of the cluster. V0442 Tau |In the region of the Pleiades cluster. V0443 Tau |In the region of the Pleiades cluster. V0444 Tau |In the region of the Pleiades cluster. Possible member V0444 Tau |of the cluster. V0445 Tau |In the region of the Pleiades cluster. V0446 Tau |The member of the Pleiades cluster. V0447 Tau |In the region of the Pleiades cluster. Not a member V0447 Tau |of the cluster. V0448 Tau |The member of the Pleiades cluster. V0449 Tau |In the region of the Pleiades cluster. Not a member V0449 Tau |of the cluster. V0451 Tau |In the region of the Pleiades cluster. Not a member V0451 Tau |of the cluster. V0452 Tau |In the region of the Pleiades cluster. Possible member V0452 Tau |of the cluster. V0453 Tau |In the region of the Pleiades cluster. Possible member V0453 Tau |of the cluster. V0454 Tau |In the region of the Pleiades cluster. Not a member V0454 Tau |of the cluster. V0455 Tau |In the region of the Pleiades cluster. V0456 Tau |In the region of the Pleiades cluster. V0457 Tau |In the region of the Pleiades cluster. V0458 Tau |In the region of the Pleiades cluster. V0459 Tau |In the region of the Pleiades cluster. V0460 Tau |In the region of the Pleiades cluster. V0461 Tau |In the region of the Pleiades cluster. Possible member V0461 Tau |of the cluster. V0462 Tau |In the region of the Pleiades cluster. Not a member V0462 Tau |of the cluster. V0463 Tau |In the region of the Pleiades cluster. V0464 Tau |In the region of the Pleiades cluster. V0465 Tau |In the region of the Pleiades cluster. V0466 Tau |In the region of the Pleiades cluster. Possible member V0466 Tau |of the cluster. V0467 Tau |In the region of the Pleiades cluster. V0468 Tau |In the region of the Pleiades cluster. V0469 Tau |In the region of the Pleiades cluster. V0470 Tau |In the region of the Pleiades cluster. Possible member V0470 Tau |of the cluster. V0471 Tau |The member of the Hyades cluster. mu alpha = + 0.117", V0471 Tau |mu delta = -0.020". V0471 Tau |EA/D/(RS + WD) + XP. d = 0.0625P. V0471 Tau |There occurs a total eclipse of the white dwarf in V0471 Tau |Min I (A = 0.04m V, 0.36m U). V0471 Tau |P var. Min I = 2440612.67083 + 0.52118321d*E V0471 Tau |(JD2440570 - 970) [06250]; Min I = 2440898.80038 + V0471 Tau |0.52118376d*E (JD2440880 - 41360), Min I = V0471 Tau |2441665.46153 + 0.52118329d*E (JD2441660 - V0471 Tau |42100) [10058]; since JD2441900 - see Table. V0471 Tau |Wave-like distorsion with the amplitude from 0.05m V0471 Tau |up to 0.27m and with the period close to the orbital V0471 Tau |one is observed in the light curve outside eclipses; V0471 Tau |sometimes there are also flares. The wave is migrating on V0471 Tau |phase in the direction of phase decreasing V0471 Tau |with a migration period of 191d [10060] or ~250d V0471 Tau |[10061]. The period of white dwarf rotation derived V0471 Tau |through X-ray observations Ppuls = 554.73s [10062]. V0472 Tau |In the region of the Pleiades cluster. V0473 Tau |P = 2.7800d? V0474 Tau |In the region of the Pleiades cluster. Not a member V0474 Tau |of the cluster. V0475 Tau |In the region of the Pleiades cluster. V0476 Tau |In the region of the Pleiades cluster. V0477 Tau |In the region of the Pleiades cluster. V0478 Tau |In the region of the Pleiades cluster. V0479 Tau |VB A (BC 8.90m, 59", 357deg); (k - b)2 = 0.40. V0480 Tau |VB A (B 10.4m, 176", 303deg). The member of the Hyades V0480 Tau |cluster. V0481 Tau |In the region of the Pleiades cluster. V0483 Tau |The member of the Hyades cluster. V0484 Tau |The member of the Hyades cluster. V0485 Tau |In the region of the Pleiades cluster. V0486 Tau |Epoch of Max (U) is given. V0486 Tau |P =/ 10.61d? [10063]. V0487 Tau |In the region of the Pleiades cluster. Not a member V0487 Tau |of the cluster. V0487 Tau |On the photograph west is at the top and V0487 Tau |south to the right. V0488 Tau |The member of the Pleiades cluster. V0489 Tau |In the region of the Pleiades cluster. V0490 Tau |In the region of the Pleiades cluster. V0491 Tau |In the region of the Pleiades cluster. Possible member V0491 Tau |of the cluster. V0492 Tau |In the region of the Pleiades cluster. Possible member V0492 Tau |of the cluster. V0493 Tau |In the region of the Pleiades cluster. V0494 Tau |In the region of the Pleiades cluster. Not a member V0494 Tau |of the cluster. V0495 Tau |In the region of the Pleiades cluster. V0496 Tau |In the region of the Pleiades cluster. V0497 Tau |In the region of the Pleiades cluster. Possible member V0497 Tau |of the cluster. V0498 Tau |In the region of the Pleiades cluster. Not a member V0498 Tau |of the cluster. V0499 Tau |In the region of the Pleiades cluster. V0500 Tau |The member of the Pleiades cluster. V0501 Tau |In the region of the Pleiades cluster. Not a member V0501 Tau |of the cluster. V0502 Tau |The member of the Pleiades cluster. V0503 Tau |In the region of the Pleiades cluster. Not a member V0503 Tau |of the cluster. V0504 Tau |In the region of the Pleiades cluster. V0506 Tau |In the region of the Pleiades cluster. Not a member V0506 Tau |of the cluster. V0507 Tau |In the region of the Pleiades cluster. V0508 Tau |In the region of the Pleiades cluster. V0509 Tau |In the region of the Pleiades cluster. V0510 Tau |In the region of the Pleiades cluster. V0511 Tau |In the region of the Pleiades cluster. V0512 Tau |In the region of the Pleiades cluster. V0513 Tau |In the region of the Pleiades cluster. V0514 Tau |In the region of the Pleiades cluster. V0515 Tau |In the region of the Pleiades cluster. V0516 Tau |In the region of the Pleiades cluster. V0517 Tau |In the region of the Pleiades cluster. Not a member V0517 Tau |of the cluster. V0518 Tau |VB B (A 14.4m; B 10", 80deg). The member of the V0518 Tau |Pleiades cluster. V0519 Tau |In the region of the Pleiades cluster. Not a member V0519 Tau |of the cluster. V0520 Tau |In the region of the Pleiades cluster. Possible member V0520 Tau |of the cluster. V0521 Tau |In the region of the Pleiades cluster. Not a member V0521 Tau |of the cluster. V0522 Tau |In the region of the Pleiades cluster. V0523 Tau |In the region of the Pleiades cluster. Not a member V0523 Tau |of the cluster. V0524 Tau |In the region of the Pleiades cluster. V0525 Tau |In the region of the Pleiades cluster. Not a member V0525 Tau |of the cluster. V0526 Tau |In the region of the Pleiades cluster. V0527 Tau |In the region of the Pleiades cluster. Not a member V0527 Tau |of the cluster. V0528 Tau |In the region of the Pleiades cluster. V0529 Tau |In the region of the Pleiades cluster. Not a member V0529 Tau |of the cluster. V0530 Tau |In the region of the Pleiades cluster. Not a member V0530 Tau |of the cluster. V0531 Tau |In the region of the Pleiades cluster. V0532 Tau |In the region of the Pleiades cluster. V0533 Tau |In the region of the Pleiades cluster. V0534 Tau |In the region of the Pleiades cluster. V0535 Tau |In the region of the Pleiades cluster. V0536 Tau |In the region of the Pleiades cluster. V0537 Tau |In the region of the Pleiades cluster. V0538 Tau |The member of the Pleiadea cluster. V0539 Tau |In the region of the Pleiades cluster. Possible member V0539 Tau |of the cluster. V0540 Tau |The member of the Pleiades cluster. V0541 Tau |The member of the Pleiades cluster. V0542 Tau |In the region of the Pleiades cluster. Not a member V0542 Tau |of the cluster. V0543 Tau |In the region of the Pleiades cluster. V0544 Tau |In the region of the Pleiades cluster. V0545 Tau |Max = 2444896.678 + 0.355d*E, M - m = 0.42P, A(V) = V0545 Tau |0.09m [10052]. The member of the Pleiades cluster. V0546 Tau |In the region of the Pleiades cluster. Not a member V0546 Tau |of the cluster. V0547 Tau |In the region of the Pleiades cluster. V0548 Tau |In the region of the Pleiades cluster. Possible member V0548 Tau |of the cluster. V0549 Tau |In the region of the Pleiades cluster. V0550 Tau |The member of the Pleiades cluster. V0551 Tau |In the region of the Pleiades cluster. V0552 Tau |In the region of the Pleiades cluster. V0553 Tau |In the region of the Pleiades cluster. Not a member V0553 Tau |of the cluster. V0554 Tau |In the region of the Pleiades cluster. V0555 Tau |In the region of the Pleiades cluster. Not a member V0555 Tau |of the cluster. V0556 Tau |In the region of the Pleiades cluster. V0557 Tau |In the region of the Pleiades cluster. Not a member V0557 Tau |of the cluster. V0558 Tau |In the region of the Pleiades cluster. V0559 Tau |In the region of the Pleiades cluster. Not a member V0559 Tau |of the cluster. V0560 Tau |In the region of the Pleiades cluster. Not a member V0560 Tau |of the cluster. V0561 Tau |In the region of the Pleiades cluster. V0562 Tau |In the region of the Pleiades cluster. V0563 Tau |In the region of the Pleiades cluster. V0564 Tau |In the region of the Pleiades cluster. V0565 Tau |In the region of the Pleiades cluster. Not a member V0565 Tau |of the cluster. V0566 Tau |In the region of the Pleiades cluster. Not a member V0566 Tau |of the cluster. V0567 Tau |In the region of the Pleiades cluster. V0568 Tau |In the region of the Pleiades cluster. V0569 Tau |In the region of the Pleiades cluster. Not a member V0569 Tau |of the cluster. V0570 Tau |In the region of the Pleiades cluster. V0571 Tau |In the region of the Pleiades cluster. V0572 Tau |In the region of the Pleiades cluster. V0573 Tau |In the region of the Pleiades cluster. V0574 Tau |In the region of the Pleiades cluster. V0575 Tau |In the region of the Pleiades cluster. V0576 Tau |In the region of the Pleiades cluster. V0577 Tau |In the region of the Pleiades cluster. V0578 Tau |In the region of the Pleiades cluster. Not a member V0578 Tau |of the cluster. V0579 Tau |In the region of the Pleiades cluster. V0581 Tau |In the region of the Pleiades cluster. V0582 Tau |In the region of the Pleiades cluster. V0583 Tau |In the region of the Pleiades cluster. V0584 Tau |In the region of the Pleiades cluster. V0585 Tau |In the region of the Hyades cluster. V0589 Tau |In the region of the Hyades cluster. V0594 Tau |In the region of the Pleiades cluster. V0595 Tau |In the region of the Pleiades cluster. V0596 Tau |In the region of the Pleiades cluster. Possible member V0596 Tau |of the cluster. V0597 Tau |In the region of the Pleiades cluster. V0598 Tau |In the region of the Pleiades cluster. V0599 Tau |In the region of the Pleiades cluster. V0600 Tau |In the region of the Pleiades cluster. V0601 Tau |In the region of the Pleiades cluster. V0602 Tau |In the region of the Pleiades cluster. Not a member V0602 Tau |of the cluster. V0603 Tau |In the region of the Pleiades cluster. V0604 Tau |In the region of the Pleiades cluster. V0605 Tau |In the region of the Pleiades cluster. V0606 Tau |In the region of the Pleiades cluster. V0607 Tau |In the region of the Pleiades cluster. V0608 Tau |In the region of the Pleiades cluster. Not a member V0608 Tau |of the cluster. V0609 Tau |In the region of the Pleiades cluster. V0610 Tau |The member of the Pleiades cluster. V0611 Tau |In the region of the Pleiades cluster. V0612 Tau |In the region of the Pleiades cluster. V0613 Tau |In the region of the Pleiades cluster. Possible member V0613 Tau |of the cluster. V0614 Tau |In the region of the Pleiades cluster. V0615 Tau |In the region of the Pleiades cluster. Not a member V0615 Tau |of the cluster. V0617 Tau |In the region of the Pleiades cluster. V0618 Tau |In the region of the Pleiades cluster. V0619 Tau |In the region of the Pleiades cluster. V0620 Tau |In the region of the Pleiades cluster. V0621 Tau |In the region of the Pleiades cluster. V0622 Tau |In the region of the Pleiades cluster. V0623 Tau |The member of the Pleiades cluster. V0624 Tau |The value of P1(A1 = 0.01m) is given in the Table. V0624 Tau |P2 = 0.017d, A2 = 0.007m. The member of the Pleiades V0624 Tau |cluster. V0625 Tau |In the region of the Pleiades cluster. V0626 Tau |In the region of the Pleiades cluster. V0627 Tau |The member of the Pleiades cluster. V0629 Tau |In the region of the Pleiades cluster. V0630 Tau |In the region of the Pleiades cluster. V0631 Tau |The member of the Pleiades cluster. V0632 Tau |The member of the Pleiades cluster. V0633 Tau |In the region of the Pleiades cluster. Not a member V0633 Tau |of the cluster. V0634 Tau |In the region of the Pleiades cluster. Not a member V0634 Tau |of the cluster. V0635 Tau |The member of the Pleiades cluster. V0636 Tau |In the region of the Pleiades cluster. Not a member V0636 Tau |of the cluster. V0637 Tau |In the region of the Pleiades cluster. V0638 Tau |The member of the Pleiades cluster. V0639 Tau |In the region of the Pleiades cluster. V0640 Tau |In the region of the Pleiades cluster. V0641 Tau |Max = 2444896.744 + 1.22d*E; M - m = 0.5P, A(V) = 0.03m V0641 Tau |[10052]. The member of the Pleiades cluster. V0642 Tau |The member of the Pleiades cluster. V0643 Tau |The member of the Pleiades cluster. V0644 Tau |The member of the Pleiades cluster. V0645 Tau |In the region of the Pleiades cluster. Possible member V0645 Tau |of the cluster. V0646 Tau |The member of the Pleiades cluster. V0647 Tau |The value V0647 Tau |of P1(A1 = 0.011m) is given in the Table. V0647 Tau |P2 = 0.070d, A2 = 0.006m. The member of the Pleiades V0647 Tau |cluster. V0648 Tau |In the region of the Pleiades cluster. V0649 Tau |In the region of the Pleiades cluster. V0650 Tau |The member of the Pleiades cluster. V0651 Tau |In the region of the Pleiades cluster. V0652 Tau |The member of the Pleiades cluster. V0653 Tau |In the region of the Pleiades cluster. Not a member V0653 Tau |of the cluster. V0654 Tau |In the region of the Pleiades cluster. Possible member V0654 Tau |of the cluster. V0655 Tau |In the region of the Pleiades cluster. V0656 Tau |In the region of the Pleiades cluster. V0657 Tau |In the region of the Pleiades cluster. Not a member V0657 Tau |of the cluster. V0658 Tau |In the region of the Pleiades cluster. V0659 Tau |In the region of the Pleiades cluster. V0660 Tau |Max = 2444896.453 + 0.23541d*E, M - m = 0.5P, A(V) = V0660 Tau |0.20m [10052]. The member of the Pleiades cluster. V0661 Tau |In the region of the Pleiades cluster. V0662 Tau |In the region of the Pleiades cluster. V0663 Tau |In the region of the Pleiades cluster. V0664 Tau |The member of the Pleiades cluster. V0665 Tau |In the region of the Pleiades cluster. Not a member V0665 Tau |of the region. V0666 Tau |In the region of the Pleiades cluster. V0667 Tau |The member of the Pleiades cluster. V0668 Tau |In the region of the Pleiades cluster. V0669 Tau |In the region of the Pleiades cluster. V0670 Tau |In the region of the Pleiades cluster. V0671 Tau |In the region of the Pleiades cluster. V0672 Tau |In the region of the Pleiades cluster. Not a member V0672 Tau |of the cluster. V0673 Tau |In the region of the Pleiades cluster. Possible member V0673 Tau |of the cluster. V0674 Tau |In the region of the Pleiades cluster. V0675 Tau |In the region of the Pleiades cluster. Not a member V0675 Tau |of the cluster. V0676 Tau |In the region of the Pleiades cluster. V0677 Tau |The member of the Pleiades cluster. V0678 Tau |In the region of the Pleiades cluster. Not a member V0678 Tau |of the cluster. V0679 Tau |The member of the Pleiades cluster. V0680 Tau |In the region of the Pleiades cluster. Not a member V0680 Tau |of the cluster. V0681 Tau |In the region of the Pleiades cluster. V0682 Tau |In the region of the Pleiades cluster. V0683 Tau |In the region of the Pleiades cluster. V0684 Tau |In the region of the Pleiades cluster. Not a member V0684 Tau |of the cluster. V0685 Tau |In the region of the Pleiades cluster. Not a member V0685 Tau |of the cluster. V0686 Tau |In the region of the Pleiades cluster. V0687 Tau |In the region of the Pleiades cluster. V0688 Tau |In the region of the Pleiades cluster. V0689 Tau |In the region of the Pleiades cluster. V0690 Tau |In the region of the Pleiades cluster. V0691 Tau |In the region of the Pleiades cluster. V0692 Tau |In the region of the Pleiades cluster. Possible member V0692 Tau |of the cluster. V0693 Tau |In the region of the Pleiades cluster. V0694 Tau |In the region of the Pleiades cluster. V0696 Tau |The member of the Hyades cluster. V0697 Tau |The member of the Hyades cluster. V0698 Tau |Type INB? V0700 Tau |The member of the Pleiades cluster. V0701 Tau |In the region of the Pleiades cluster. V0702 Tau |In the region of the Pleiades cluster. V0703 Tau |The member of the Pleiades cluster. V0705 Tau |In the region of the Pleiades cluster. V0706 Tau |In the region of the Pleiades cluster. V0707 Tau |In the region of the Pleiades cluster. V0709 Tau |In the region of the Pleiades cluster. V0710 Tau |VB A (B 16m, 3.5", 180deg). V0711 Tau |VB A (B 8.83m, A = 8.023", E = 0.18, Porb = 2101 yr); V0711 Tau |SB2 (Porb = 2.83774d [10070]). V0711 Tau |Migration period of the distortion wave is about V0711 Tau |10.5 yr [10072]. V0711 Tau |The range of combined light variation is given. V0712 Tau |In the region of the Pleiades cluster. V0713 Tau |In the region of the Pleiades cluster. V0714 Tau |In the region of the Pleiades cluster. V0715 Tau |In the region of the Pleiades cluster. V0716 Tau |In the region of the Pleiades cluster. V0717 Tau |In the region of the Pleiades cluster. V0718 Tau |In the region of the Hyades cluster. V0725 Tau |SB1 (Porb = 110.8d [10076]). V0725 Tau |X-ray outbursts occur periodically near V0725 Tau |the periastron passages of the pulsar with P = Porb. V0725 Tau |The amplitude of the corresponding variations of V0725 Tau |visual brightness of the system A(V) = 0.03m. The period V0725 Tau |of pulsar rotation Prot var [10077]. V0725 Tau |Prot = 104.17s (JD2442531), 103.806s (JD2442728), V0725 Tau |103.882s (JD2443505), 103.8402s (JD2443620) V0725 Tau |[10074]; 103.647s (JD2444521), 103.423s V0725 Tau |(JD2445292), 103.3429ss(JD2445623) [10078]. V0726 Tau |Min II 11.2. V0727 Tau |In the region of the Pleiades cluster. V0728 Tau |In the region of the Pleiades cluster. Not a member V0728 Tau |of the cluster. V0729 Tau |Max = 2439024.46 + 152.35d*E (JD2438680 - 39415); V0729 Tau |Max = 2440127.78 + 313.86d*E (JD2439415 - 40510). V0729 Tau |H2O maser. V0732 Tau |In the region of the Pleiades cluster. V0733 Tau |In the region of the Pleiades cluster. V0734 Tau |In the region of the Pleiades cluster. V0735 Tau |In the region of the Pleiades cluster. V0736 Tau |In the region of the Pleiades cluster. V0737 Tau |In the region of the Pleiades cluster. V0738 Tau |In the region of the Pleiades cluster. The chart in [08559] V0738 Tau |is wrong. V0739 Tau |In the region of the Pleiades cluster. V0740 Tau |In the region of the Pleiades cluster. V0741 Tau |In the region of the Pleiades cluster. V0742 Tau |In the region of the Pleiades cluster. V0743 Tau |In the region of the Pleiades cluster. V0744 Tau |In the region of the Pleiades cluster. V0746 Tau |In the region of the Pleiades cluster. V0747 Tau |In the region of the Pleiades cluster. V0748 Tau |In the region of the Pleiades cluster. V0749 Tau |In the region of the Pleiades cluster. V0750 Tau |In the region of the Pleiades cluster. V0751 Tau |In the region of the Pleiades cluster. V0752 Tau |In the region of the Pleiades cluster. V0753 Tau |In the region of the Pleiades cluster. Not a member V0753 Tau |of the cluster. V0754 Tau |In the region of the Pleiades cluster. V0755 Tau |In the region of the Pleiades cluster. V0756 Tau |In the region of the Pleiades cluster. V0757 Tau |In the region of the Pleiades cluster. V0758 Tau |In the region of the Pleiades cluster. Not a member V0758 Tau |of the cluster. V0759 Tau |In the region of the Pleiades cluster. V0760 Tau |In the region of the Pleiades cluster. V0761 Tau |In the region of the Pleiades cluster. Not a member V0761 Tau |of the cluster. V0762 Tau |In the region of the Pleiades cluster. Not a member V0762 Tau |of the cluster. V0763 Tau |In the region of the Pleiades cluster. V0764 Tau |In the region of the Pleiades cluster. V0765 Tau |In the region of the Pleiades cluster. V0767 Tau |In the region of the Pleiades cluster. V0768 Tau |In the region of the Pleiades cluster. V0769 Tau |In the region of the Pleiades cluster. V0770 Tau |In the region of the Pleiades cluster. V0771 Tau |In the region of the Pleiades cluster. V0772 Tau |In the region of the Pleiades cluster. V0773 Tau |There are also quasisinusoidal light variations with V0773 Tau |P = 3.43d and A(V) = 0.13m [10056]. V0774 Tau |VB A (B 6.96m, G5IV, 66.8", 315deg). V0775 Tau |The member of the Hyades cluster. V0776 Tau |VB A (B 7.5m, 1.4", 333deg, 1958; C 8.7m, 77.2", 233deg, V0776 Tau |1925); SB1 (Porb = 57.25d). The member of the V0776 Tau |Hyades cluster. V0777 Tau |VB A (B 8.12m V, 0.0088", 173.2deg, 1980.6). V0777 Tau |The member of the Hyades cluster. V0778 Tau |Min II 17.0. P var. Min I = 2438680.546 + 0.434842d*E V0778 Tau |(JD2436528 - 38841); Min I = 2439765.488 + 0.434846d*E V0778 Tau |(JD2439559 - 41031); since JD2440129 - see Table. V0780 Tau |VB A (B 15.8m V, 0.3", 310deg, 1974); mu = 0.364", V0780 Tau |P = 163deg. V0781 Tau |Min II 9.3. V0782 Tau |In the region of the Pleiades cluster. V0783 Tau |In the region of the Pleiades cluster. V0784 Tau |In the region of the Pleiades cluster. V0785 Tau |The member of the Pleiades cluster. V0787 Tau |In the region of the Pleiades cluster. V0788 Tau |In the region of the Pleiades cluster. V0789 Tau |The member of the Pleiades cluster. V0790 Tau |The member of the Pleiades cluster. V0791 Tau |In the region of the Pleiades cluster. V0792 Tau |Near V752 Tau. Identical to it? V0792 Tau |In the region of the Pleiades cluster. V0793 Tau |The member of the Pleiades cluster. V0794 Tau |In the region of the Pleiades cluster. Not a member V0794 Tau |of the cluster. V0795 Tau |In the region of the Pleiades cluster. V0796 Tau |The member of the Pleiades cluster. V0797 Tau |In the region of the Pleiades cluster. Not a member V0797 Tau |of the cluster. V0798 Tau |In the region of the Pleiades cluster. V0799 Tau |In the region of the Pleiades cluster. V0800 Tau |In the region of the Pleiades cluster. V0801 Tau |In the region of the Pleiades cluster. V0802 Tau |In the region of the Pleiades cluster. V0804 Tau |In the region of the Pleiades cluster. V0805 Tau |The member of the Hyades cluster. V0807 Tau |VB A (B = GH Tau, 21.4", 193deg). V0808 Tau |Porb = 11.93d. The member of the Hyades cluster. V1144 Tau |SB, Porb = 13.88d. V1148 Tau |Type LBV: is also possible. SB, Porb = 2.2075d. V1152 Tau |Type E: with P = 11.080d is also possible. V1161 Tau |Variability needs confirmation. V1212 Tau |Dwarf nova in Taurus. alf Tau |VB A (B 13.5m, M2V, 31", 110deg). alf Tau |The star is surrounded by an infrared emission envelope alf Tau |with the diameter of about 10". In the region of the alf Tau |Hyades cluster. zet Tau |Min II 3.05. tet 2 Tau |VB A (B 4.85m, 0.02077", 19.6deg, 1980.59); SB1 (Porb = tet 2 Tau |140.728D, E = 0.75 [10087]). The value of P1(A1 = 0.017m B) tet 2 Tau |is given in the Table. P1 var. Later P1 = 0.07541d tet 2 Tau |(A1 = 0.023m B), P2 = 0.0831d (A2 = 0.013m B). Possibly tet 2 Tau |eclipsing with the elements: tet 2 Tau |Min = 2445358.38 + 140.734d*E, A = 0.02m B. tet 2 Tau |The member of the Hyades cluster. lam Tau |Min II 3.54. Triple system. The eclipsing system rotates lam Tau |around the third component with P = 33.025d [10090]. lam Tau |In the region of the Hyades cluster. rho Tau |The member of the Hyades cluster. ups Tau |VB A (B 6.5m, 0.020"). The member of the Hyades cluster. U Tel |P var. Before JD2421000 Max = 2420992 + 439.13d*E [00001]; U Tel |since JD2423000 - see Table. RR Tel |During 1889 - 1930 12m - 14m pg (according to [00625], RR Tel |irregular variations; according to [00017], RR Tel |Max = 2411490 + 384d*E, with irregularities). During RR Tel |1930 - 1944 12.5m - 16.5m pg, Max = 2430145 + 386.73d*E RR Tel |[01649]; after 1938 an increase of mean brightness RR Tel |and of the amplitude was noted. An outburst from RR Tel |14m to 7m in October, 1944. In Max, 6.5m - 7.5m pg, RR Tel |during JD2431500 - 33000; after JD2433100 began RR Tel |to decline its mean brightness. Near the Max of the RR Tel |outburst no periodic variations was noted. During RR Tel |JD2441426 - 44899 5.06m - 6.74m J, P = 387d [09989], RR Tel |M - m = 0.5P; Min (V) = 2442551 + 374.2d*E (1961 - 1981), RR Tel |Delta(V) = 0.25m for periodic changes [10029]; RR Tel |9.8m - 10.7m B, P = 395d (JD2443500 - 45500) [10030]. RR Tel |In the Max of the outburst the spectrum was F5 RR Tel |without emissions. During the brightness decline a RR Tel |rich emission spectrum was formed with lines of RR Tel |hydrogen, forbidden lines of metals in high stages RR Tel |of ionization, etc. Since the 1970-ies TiO absorption RR Tel |bands are being noted. Radio source, soft X-ray source. RS Tel |Semiregular variations, P = 45.8d [08140]. IR excess. RV Tel |VB (0.6", 294deg, 1946). d = 0.02P. ST Tel |The chart in [06286] is wrong. SZ Tel |Possibly identical with the star alpha = 18h 13m 16s, SZ Tel |delta = -53deg 39.2', 1950.0 (RR, 15m - 16.5m pg) [10032]. SZ Tel |In the region of the globular cluster NGC 6584. TT Tel |In the region of the globular cluster NGC 6584. TU Tel |In the region of the globular cluster NGC 6584. TV Tel |In the region of the globular cluster NGC 6584. TW Tel |In the region of the globular cluster NGC 6584. The chart TW Tel |in [06286] is wrong. TX Tel |In the region of the globular cluster NGC 6584. The chart TX Tel |in [06286] is wrong. UY Tel |VB. AG Tel |nf star of a pair. AK Tel |Very red. AX Tel |[A/H] = -0.7. BL Tel |The depth of Min II - 0.1m pg. BL Tel |Semiregular variability of pulsational character BL Tel |(7.09m - 7.26m V) is observed outside eclipses; sometimes BL Tel |it may be represented by P = 65.1d, but sometimes (1969) BL Tel |it cannot be traced. BO Tel |[A/H] = -0.3. CK Tel |VB B (A 15.0m). DZ Tel |sf star of a pair. FR Tel |D >= 0.23P. Min II 14.0? GH Tel |P ~10.342d is possible. GM Tel |VB A. GR Tel |The chart in [06286] is wrong. GY Tel |Min II 12.0. HH Tel |P var slightly. HO Tel |Min II 8.67. HR Tel |EW type with twice longer P is possible. IL Tel |The elements need confirmation. IQ Tel |Min II 12.7. KK Tel |B - V: +0.6m: (Min light). KN Tel |VB A (B 16m sf). LW Tel |Possibly identical to NSV10695. MT Tel |mu alpha = -0.0127S, mu delta = -0.109". MT Tel |[Fe/H] = -1.82. Delta(S) = 9.9. MV Tel |EW type with twice longer P is possible. MZ Tel |EW type with twice longer P is possible. NN Tel |Min II 15.5. NP Tel |Min II 13.3. NS Tel |Min II 9.4. NV Tel |Min II 9.0. OQ Tel |sf star of a pair. PR Tel |Min II 11.35. Radio source PKS 1925 - 524. PR Tel |Hbeta fluctuates on ~5 min time scale. PS Tel |V39 (NGC 6584). Probably non-member of the cluster. PS Tel |P = 0.1422d or 0.1657d is possible. PT Tel |V27 (NGC 6584). Cluster non-member. PU Tel |V24 (NGC 6584). Cluster non-member. PV Tel |SB2. PX Tel |V15 (NGC 6584). Cluster non-member. PZ Tel |SB2. QZ Tel |The variability may be due to the fainter (B) component. V0337 Tel |Type EW: is also possible. R Tri |P var. Max = 2412167 + 267.3d*E (JD2412000 - 16000); R Tri |Max = 2416972 + 262.6d*E (JD2416000 - 20000); R Tri |since JD2420000 - see Table. Maser (H2O). S Tri |P var. Max = 2418541 + 248.9d*E (JD2418000 - 31000); S Tri |since JD2431000 - see Table. T Tri |P var. Max = 2420535 + 320.6d*E (JD2420000 - 27000); T Tri |since JD2427000 - see Table. U Tri |Delta(S) = 1.3. V Tri |Min II 11.0. X Tri |VB A (B 13.3m, 6.7", 55.3deg, 1952). Usual brightness in X Tri |Max 8.88. d = 0.013P; Min II 9.07. According to [10043], X Tri |a two-peaked flare-like event of 35 min duration X Tri |(Delta(V) = 0.33m) was observed at JD2445594.4550. X Tri |P var. Min = 2422722.269 + 0.9715342d*E X Tri |(JD2422700 - 26600); Min = 2426946.508 + 0.9715390d*E X Tri |(JD2426600 - 33400); Min = 2433504.397 + 0.9715290d*E X Tri |(JD2433400 - 35500); X Tri |Min = 2435687.422 + 0.9715352d*E (JD2435500 - 39200); X Tri |Min = 2439375.373 + 0.9715277d*E X Tri |(JD2439200 - 42500) [07603]; since JD2442500 - see Table. Y Tri |Var No.2 (M33). VB A (B 17.28m B, 26.4" np). RS Tri |VB A (B 11.98m, 6.0", 214deg, 1962). RS Tri |d = 0.016P; Min II 10.4, Min II - Min I = 0.56P. RU Tri |VB A (B 12m, 21.8", 88deg). Min II 11.8:. RW Tri |The depth of Min I 1.12m - 2.21m. RW Tri |D = 0.052P - 0.086P, d ~0.03P. P var? [03434,09858,9859]. RW Tri |Strong fluctuations of light outside eclipses. the lower RW Tri |the brightness outside the eclipse, the deeper the Min. RW Tri |In J, K light Min II of 0.16m J depth was found at the RW Tri |phase 0.50P [10053]. Flat spectrum of the accretion disc RW Tri |with emission lines. RX Tri |Max = 2426577 + 192d*E (JD2426500 - 31800); RX Tri |since JD2432800 - see Table. According to [04029], RX Tri |P = 100d? RY Tri |Red. ST Tri |Min II 14.5. SW Tri |Blazhko effect is possible. SY Tri |Blazhko effect is possible. TT Tri |In the region of the galaxy M 33. TZ Tri |ADS 1697 A (B 6.72m, F6V, SB2, Porb = 2.2365d, TZ Tri |3.9", 71deg, 1973); SB2 (P = 14.732d). Secondary TZ Tri |variations on ~100d time scale. H and K CaII emission was TZ Tri |noted only for one of the two G-stars. alf Tri |SB (Porb = 1.767 d). R TrA |SB? U TrA |For moments of Max0 (fundamental mode) see Table. U TrA |Max1 (first overtone) = 2443266.05 + 1.824881d*E. RR TrA |Min II 10.60, dII = 0.025P. RW TrA |(k - b)2 = 0.30. Delta(S) = 1. SU TrA |The chart in [06286] is wrong. TW TrA |VB. TY TrA |The chart in [06286] is wrong. UW TrA |The chart in [06286] is wrong. UZ TrA |The chart in [06286] is wrong. XX TrA |The chart in [06286] is wrong. XY TrA |The chart in [06286] is wrong. AS TrA |Min II 15.7. BH TrA |According to [04637], L type. CI TrA |Possibly P < 0.3d. DI TrA |The chart in [06286] is wrong. DV TrA |Three Max and three Min are observed during a cycle. DV TrA |Max1 (phi = 0.0P) 13.2m; Max2 (phi = 0.2P) 14.2m; Max3 DV TrA |(phi = 0.6P) 13.5m. Min1, Min2, Min3 ~16.0m. DZ TrA |The chart in [06286] is wrong. EH TrA |Shallow Min II is possible. EK TrA |n star of a pair. EK TrA |For the mean cycle between normal maxima see Table. The EK TrA |mean cycle between supermaxima 442.1d (JD2435200 - 39700), EK TrA |551.5d (JD2439700 - 44050). Superhumps (delta(M) = 0.26m V) EK TrA |with P = 0.06492d, M - m = 0.26P [09945]. EL TrA |Min II 10.9. EM TrA |Min II 10.4. EN TrA |According to [07934], RV: type. EP TrA |Min II 9.5. EQ TrA |Min II 9.0. EQ TrA |P var. Min = 2416267.614 + 2.709220d*E (JD2416000 - 29000); EQ TrA |since JD2429000 - see Table. ER TrA |P > 220d. FH TrA |The elements need confirmation. FK TrA |The elements need confirmation. FM TrA |P >= 220d. GN TrA |Min II 12.0. HP TrA |Deep Min II. The elements need improvement. HV TrA |Min II? 14.8. Min II - Min I = 0.55P. IM TrA |P >= 150d. Epoch of Min is given. IW TrA |Min II 14.5:. The elements need confirmation. KX TrA |2U 1639-62? P.K.326 -10deg 1. Gas velocities up to KX TrA |5000 km/s [09958]. KY TrA |TrA X-1 = A1524-61. KZ TrA |4U 1626-67. Lx/Lopt ~2000. VB B (A 14.9m; B25", 189deg). KZ TrA |Barycentric period parameters for pulses [04534]: Min = KZ TrA |JED 2443931.2394789; P = 7.6776762s, DP/dt = KZ TrA |(-4.95 +-0.02)*10**(-11). Delta(m) pulse = 0.02m - 0.17m. KZ TrA |Porb = 2491.06s or 2492.32s [04558]. KZ TrA |Flares with Delta(m) up to 0.4m with intervals ~20 min KZ TrA |correlated with X-ray flares [04536]. LM TrA |The chart in [08661] is wrong. LP TrA |VB A (B 11.5m, 25", 123deg; C 12.0m, BC 6"). T Tuc |P var. Max = 2410138 + 250.76d*E (JD2410000 - 14400); T Tuc |Max = 2414900 + 248.88d*E (JD2414400 - 22000); T Tuc |Max = 2432160 + 250.00d*E (JD2422900 - 35000); T Tuc |since JD2437700 - see Table. U Tuc |In the region of the Small Magellanic Cloud. U Tuc |SMS non-member. U Tuc |P var. Max = 2421190 + 258.12d*E (JD2412600 - 22000); U Tuc |Max = 2427487 + 262.83d*E (JD2422000 - 28000); U Tuc |Max = 2437808 + 257.70d*E (JD2428000 - 39150); U Tuc |since JD2440900 - see Table. V Tuc |In the region of the Small Magellanic Cloud. V Tuc |SMS non-member. V Tuc |The depth of Min II 0.11m. W Tuc |(k - b)2 = 0.09, Delta(S) = 7:. P var? RR Tuc |In the region of the Small Magellanic Cloud. RR Tuc |VB A (B 17m, 6", 90deg). RV Tuc |In the region of the Small Magellanic Cloud. VB. SS Tuc |In the region of the Small Magellanic Cloud. HV 1877. SS Tuc |Earlier was erroneously identifded with HV 1887. SU Tuc |In the region of the Small Magellanic Cloud. HV 1922. SU Tuc |According to [09980], alternatively may be identical to SU Tuc |HV 1920. SX Tuc |In the region of the Small Magellanic Cloud. VB (B 16m? P). SY Tuc |In the region of the Small Magellanic Cloud. Min II 15.4. TV Tuc |In the region of the Small Magellanic Cloud. TV Tuc |The variable's position in 2' to the north TV Tuc |of CPD -73deg 64 [09980] makes it impossible to identify TV Tuc |it with HV 2041. TZ Tuc |In the region of the Small Magellanic Cloud. TZ Tuc |SMS non-member. TZ Tuc |VB A (B 13m sp). UW Tuc |In the region of the Small Magellanic Cloud. UW Tuc |SMC non-member. UX Tuc |In the region of the Small Magellanic Cloud. UX Tuc |SMS non-member.In the neighbourhood OF 47 Tuc; probably UX Tuc |cluster non-member. P var. [Fe/H] = -1.8. YY Tuc |The elements need improvement; current elements with the YY Tuc |epoch from [07984] are given. YY Tuc |(k - b)2 = 0.03. Delta(S) = 8:. AD Tuc |In the region of the Small Magellanic Cloud. AD Tuc |SMS non-member. Delta(S) = 4.9. AF Tuc |In the region of the Small Magellanic Cloud. SMS AF Tuc |non-member. AH Tuc |In the region of the Small Magellanic Cloud. SMS AH Tuc |non-member. P var. AI Tuc |In the region of the Small Magellanic Cloud. SMS AI Tuc |non-member. In the region of the globular cluster NGC 362. AI Tuc |P var. AK Tuc |In the region of the Small Magellanic Cloud. SMS AK Tuc |non-member. P var. AL Tuc |In the region of the Small Magellanic Cloud. SMS AL Tuc |non-member. AM Tuc |The elements should be checked. AM Tuc |[Fe/H] = -1.82. Delta(S) = 9.9. AO Tuc |The elements need improvement. Delta(S) = 5. AP Tuc |In the region of the Small Magellanic Cloud. SMS AP Tuc |non-member. AQ Tuc |In the region of the Small Magellanic Cloud. SMS AQ Tuc |non-member.In the region of the globular cluster 47 Tuc. AQ Tuc |Min II 10.48. AR Tuc |In the region of the Small Magellanic Cloud. SMS AR Tuc |non-member. AU Tuc |In the region of the Small Magellanic Cloud. SMS AU Tuc |non-member. AV Tuc |In the region of the Small Magellanic Cloud. SMS AV Tuc |non-member. BD Tuc |In the region of the Small Magellanic Cloud. SMS BD Tuc |non-member. BE Tuc |In the region of the Small Magellanic Cloud. BF Tuc |In the region of the Small Magellanic Cloud. [A/H] = -0.7. BG Tuc |In the region of the Small Magellanic Cloud. SMS BG Tuc |non-member. BH Tuc |In the region of the Small Magellanic Cloud. VB A BH Tuc |(B 14.28m, 10" n). BS Tuc |(k - b)2 = 0.10. BZ Tuc |P var. Max = 2429849.448 + 127.78d*E (JD2410000 - BZ Tuc |35100) [03641]; Max = 2441193.541 +127.27d*E BZ Tuc |(JD2435100 - 43500) [A.M. van Genderen, AsAp Suppl 52, BZ Tuc |423, 1983]; since JD 2443500 - see Table. CF Tuc |In the region of the Small Magellanic Cloud. SMS CF Tuc |non-member. Soft X-ray source. Distortion CF Tuc |wave. Delta(m) = 0.057m [10065]. Min II 7.52. DX Tuc |Type RRC: is also possible. tet Tuc |For the period of the main oscillation (A = 0.0132m) see tet Tuc |Table. Other instable frequences were also noted. R UMa |Maser (H2O). S UMa |S 1.5/6 e. P var. Max = 2398325 + 224.51d*E S UMa |(JD2394000 - 2405000); Max = 2405290 + 230.20d*E S UMa |(JD2405000 - 10500); Max = 2417530 + 223.96d*E S UMa |(JD2410500 - 23500); Max = 2426324 + 228.53d*E S UMa |(JD2423500 - 28800); since JD2428800 - see Table. T UMa |Maser (H2O). W UMa |ADS 7494 A (B 12.35m, 6.5", 44deg, 1963). W UMa |dI = 0.037P; Min II 8.43, dII = 0.028P. W UMa |Soft X-ray source. LX/Lbol = 1.7*10**(-4). W UMa |P var. Min I = 2420980.8093 + 0.333638880d*E W UMa |(JD2416000 - 21000); Min I = 2420980.8093 + W UMa |0.333636993d*E (JD2421000 - 33000) [01760]; W UMa |Min I = 2435918.4169 + 0.33363832d*E (JD2433000 - 41000) W UMa |[05327]; since JD2441000 - see Table. The light curve shape, W UMa |including depths of minima, var. A moving wave with W UMa |Delta(m) = 0.025m y and P ~1100d [10067] was noted. A W UMa |flare (Delta(m) = 1.5m, lambda 3300 A, W UMa |delta(lambda) = 50 A, JD2438511.7, W UMa |delta(t) = 7 min) was announced [05788]. The system W UMa |contains gaseous streams, dark spots on the surface of W UMa |the components. H and K CaII emission. Z UMa |Usually 2 Max and 2 Min during a cycle. RV UMa |P var. Max = 2417861.434 + 0.4680618d*E RV UMa |(JD2417800 - 25000); Max = 2425053.675 + 0.4680654d*E RV UMa |(JD2425000 - 29000) [00188]; RV UMa |Max = 2438459.945 + 0.468062d*E (JD2429000 - 40000) [03506]; RV UMa |since JD2440000 - see Table. Blazhko effect, Pi = 92.12d RV UMa |(JD2436229 - 38114) [09835]. Pi var. [Fe/H] = -1.04; RV UMa |Delta(S) = 3.5. RW UMa |DI < 0.08P; Min II 10.34, DII = 0.10P. RW UMa |[Fe/H]A = -0.1, [Fe/H]B = -1.0. P var? RW UMa |Distortion wave, A = 0.11m V. SU UMa |The cycle of normal maxima 5d - 35d [09782,03791]. SU UMa |Three different mean values of the mean cycle of SU UMa |supermaxima change each other being active at different SU UMa |time intervals: P1 = 161.5d; P2 = 203.9d; P3 = 248.1d SU UMa |(<P> = 201.7d) [09276]. Porb = 2.06d/N (N = 26, 27, 28) SU UMa |or 3.1h. Surrounded by a faint halo (28' diameter) of soft SU UMa |X-ray sources. SW UMa |SB. Superior conjunction of the accretion disc SW UMa |T = 2445376.8601 + 0.0567433d*E [09836]. SX UMa |P var strongly. Before JD2418800 SX UMa |Max = 2416200.486 + 0.3071148d*E; SX UMa |Max = 2418800.213 + 0.3071345d:*E (JD2418800 - 22500) SX UMa |[00001]; Max = 2422653.5032 + 0.30711855d*E SX UMa |(JD2422500 - 26000) [10083]; Max = 2426400.418 + SX UMa |0.3071555d*E (JD2426000 - 29500); Max = SX UMa |2430000.250 + 0.3071301d*E (JD2429500 - 34000), SX UMa |Max = 2438508.751 + 0.3071363d*E (JD2434000 - 39000); SX UMa |since JD2441500 - see Table. [Fe/H] = -1.82, SX UMa |Delta(S) = 9.9. SZ UMa |mu alpha = -0.4853s, mu delta = +0.148". TU UMa |P var [03506]. [Fe/H] = -1.05, Delta(S) = 7.6. TW UMa |d = 0.002P; Min II 12.3:. TX UMa |Min II 7.13. P var. Min I = 2416426.801 + 3.063297d*E TX UMa |(JD2416000 - 22000); Min I = 2427926.492 + 3.063337d*E TX UMa |(JD2424200 - 30000); Min I = 2433440.431 + 3.063300d*E TX UMa |(JD2430000 - 38000) [09839]; since JD2438000 - see Table. TY UMa |P var, non-linear term: +6.4d*10**(-11)*E**2. TY UMa |dI = 0.05P, dII = 0.00P. The light curve shape var. TY UMa |12.10 <= Min I <= 12.14, 12.06 <= Min II <= 12.12. UX UMa |The shape of the eclipse light curve, the UX UMa |mean level of light outside eclipses, the depth of UX UMa |Min var. Deviations from the tabulated elements may UX UMa |reach +-0.002d. Rapid brightness oscillations UX UMa |(28.54s <= P <= 30.02s) are sometimes observed [07304]. UX UMa |Soft X-ray source. UY UMa |Min II 12.9. VV UMa |Min II 10.26. P var. Min I = 2439245.408 + 0.6873793d*E VV UMa |(JD2425600 - 40200) [09843]; Min I = 2440768.6280 + VV UMa |0.687367d*E (JD2440200 - 42700); since JD2442700 - see VV UMa |Table. VX UMa |Maser (H2O). WX UMa |Mu alpha = -0.4094s, mu delta = +0.955", VB B WX UMa |(A = BD +44deg 2051, dM2, 8.74m V; B 28", 133deg; WX UMa |common mu). Soft X-ray source. LX/LV = 0.095. XY UMa |Mu alpha = -0.0055s, mu delta = -0.175". P var. XY UMa |Non-linear term: +2.77d*10**(-11)*E**2. XY UMa |The brightness outside eclipses var by 0.16m V. The depth XY UMa |of Min I is 0.48m - 0.67m, that of Min II is 0.19m. XY UMa |Migrating wave. XZ UMa |Min II 10.2. P var? Min = 2444986.445 + 1.2223105d*E XZ UMa |(JD2414990 - 45000); since JD2445000 - see Table. AA UMa |Min II 11.53, Max II 10.94. The elements should AA UMa |be checked. AC UMa |VB B (A = BD + 65G671, 9.97m V, B-V = +0.50m; B 19", AC UMa |114deg, 1957). The chart in [08953] is wrong. AD UMa |Blazhko effect is possible. Pi = 35d - 40d, AD UMa |delta(A) = 0.2m. AE UMa |The fundamental mode P0 is given in the Table. AE UMa |P1 = 0.066527d, Pbeat = 0.293616d [09869]. AE UMa |Max 10.86 - 11.10, Min 11.46 - 11.52. AF UMa |d = 0.05P. AK UMa |The elements need improvement. AN UMa |The epoch of Min for periodic (P = Porb) light variations AN UMa |with A <= 1m B is given. Min II is present. B - V = 0.0 AN UMa |in Max light, +0.5 during an eclipse; U - B = -1.1. AN UMa |Circular polarization in B light -9% to -35%; linear AN UMa |polarization 0% - 13% with a sharp Max near Max light. AN UMa |Rapid changes (A = 0.03m, f = 0.4 - 0.8 Hz). The mean AN UMa |light level and the light curve shape var. During the low AN UMa |state (B ~19m) the light variability with porb disappears, AN UMa |emission lines occur only during 10% of Porb, IR excess is AN UMa |noted. Soft X-ray source, var. Emissions of H, HeI, AN UMa |He II, NIII, FeII. AW UMa |dI = 0.06P:; Min II 7.08, dII = 0.11P. AW UMa |The light curve shape var. AW UMa |P var. Min I = 2442150.4385 + 0.43873234d*E AW UMa |(JD2438000 - 42200); since JD2442200 - see Table. AX UMa |P var. Max = 2435951.354 + 0.53510d*E (JD2435900 - 38200) AX UMa |[04375]; during JD2445000 - 45900 - see Table. BE UMa |d = 0.006P. Outside eclipses var BE UMa |14.8m <= B <= 16.0m (reflection effect). The depth of BE UMa |eclipses for lambda lambda 3330 - 3700 A is greater than BE UMa |4.3m,that for lambda lambda 5265 - 6005 A is 1.5m. BG UMa |Min II 10.93. Alternative type EW. BH UMa |Min II 12.3. BI UMa |Min II 15.8. BK UMa |[Fe/H] = -1.29, Delta(S) = 6.6. BL UMa |Min II 16.2. BM UMa |The depth of Min II 0.80m. BN UMa |[Fe/H] = -1.65, Delta(S) = 8.9. BP UMa |D <= 0.04P. The elements need confirmation. CE UMa |In the region of the cluster of galaxies Abell 1213. CE UMa |SN 1966 omicron? CF UMa |Groombridge 1830 B (A = BD +38deg 2285, V = 6.45m, CF UMa |B - V = +0.75m, G8 subdwarf, mu alpha = + 0.339s, CF UMa |mu delta = -5.81"; B 2", 165deg). A possible flare on CF UMa |February 27, 1968. A brightening of the combined light by CF UMa |0.6m pg on April 27, 1939 [09881]. Maybe the object does CF UMa |not exist [09882]. CH UMa |X-ray source 1E 1003 +67. LX/Lopt = 0.04. CM UMa |P var? CQ UMa |The epoch of Max in U and B light CQ UMa |coinciding with that of Min in V light is given. CQ UMa |A(U) = 0.06m, A(B) = 0.06m. CR UMa |The elements for Max in U light are given. In B and V CR UMa |bands no periodicity is apparent. A(U) = 0.03m. CW UMa |Mu = 0.27", P = 300deg. DF UMa |ADS 8242A (B 11.4m, 1.8", 60deg, 1960). DF UMa |The data for combined brightness are given in the Table. DF UMa |SB1, Porb = 1.033824d. Mu alpha = +0.0131s, DF UMa |mu delta = -0.038". Besides rapid variations (<V> = 10.14m, DF UMa |Delta(V) = 0.05m), long term variations are possible. DG UMa |Blazhko effect is possible. DK UMa |Soft X-ray source, lg Lx/Lv = -3.5. [Fe/H] = -0.38. DL UMa |Eclipses with P = 0.42d [04706]. DM UMa |SB1 (Porb = 7.492d). DM UMa |Min = 2444026.97 + 7.478d*E (1979 - 1982); DM UMa |1981 - 1984 - see Table. Two Min in the light curve in DM UMa |1981 - 1982. DN UMa |ADS 8347 ABC (A 7.2m vis; B 9.0m vis, 0.121", 142.0deg, DN UMa |1981.5; C 8.3m vis, 4.0", 42deg, 1980; D = BS 4561, DN UMa |A1pCrEuSr:, V = 7.03m, B - V = +0.01m, 63.0", 114deg). DN UMa |The range of combined brightness for the three components DN UMa |is given. It is not known which of the components varies. DN UMa |The component D was used as a comparison star. DN UMa |Min II 6.73, Min II - Min I = 0.504P. GM UMa |SB, discrepant Porb = 3.2424d. HH UMa |Type EW: is also possible. HN UMa |Type DSCT: is also possible. HU UMa |VB A (B = GSC 3014.0222 = L265-581, 24", 250 deg, common proper HU UMa |motion). II UMa |Type RR: is also possible. eps UMa |SB (P=4.15A). Interferometric binary? (0.053", 94.5deg, eps UMa |1975.4). In 1976 - 1983 attempts to resolve the binary eps UMa |interferometrically were not successful. eps UMa |In the UMa moving cluster; mu alpha = +0.0131s, eps UMa |mu delta = -0.010". ups UMa |ADS 7534 A (B 11.5m, 11.3", 295deg, common mu). ups UMa |mu alpha = -0.0382s, mu delta = -0.156". The light curve ups UMa |shape and A var. R UMi |H2O maser. S UMi |P var. Max = 2422604 + 321.9d*E (JD2413000 - 23000); S UMi |Max = 2432200 + 331.5d*E (JD2423000 - 32800); S UMi |Max = 2436080 + 322.5d*E (JD2433000 - 37000); S UMi |Max = 2439011 + 326.5d*E (JD2437000 - 41500); S UMi |since JD2441500 - see Table. T UMi |P var. Max = 2428332 + 315.48d*E (JD2416500 - 29500); T UMi |Max = 2436415 + 310.05d*E (JD2429500 - 37200); T UMi |Max = 2442389 + 315.5d*E (JD2437200 - 43600); since T UMi |JD2443600 - see Table. U UMi |P var. Max = 2416975 + 323.1d*E (JD2416500 - 21000); U UMi |Max = 2428804 + 331.3d*E (JD2421000 - 29780) [00001]; U UMi |Max = 2429789 + 320.6d*E (JD2429780 - 34600) [00960]; U UMi |Max = 2434600 + 331d*E (JD2434600 - 36300); U UMi |Max = 2437853 + 322.6d*E (JD2436300 - 39000); since U UMi |JD2439000 - see Table. V UMi |Mean brightness var with P2 = 760d. W UMi |Min II 8.66; d = 0.02P. P var? Non-linear term in the W UMi |elements is possible: -7.7d*10**(-10)*E**2. X UMi |P var? Max = 2424224 + 343d*E (JD2423800 - 25100) X UMi |[00684]; since JD2438100 - see Table. RR UMi |SB (Porb = 749.4d [09896]). RT UMi |Min II 10.86. RU UMi |Min II 10.20. RZ UMi |Min II 13.5. SZ UMi |Variability needs confirmation. alf UMi |VB A (B 8.20m, F3V, 18.3", 218deg); SB1 (Porb = 10969d, alf UMi |E = 0.655 [09904]). P var. There is a non-linear term in alf UMi |the elements: +1.9877d*10**(-7)*E**2. The amplitude of alf UMi |light and radial velocity variation decreased in 1982. alf UMi |A(V) = 0.04m (1984). gam UMi |P var. Max = 2424301.78 + 0.14335d*E [10097]; Max = gam UMi |2427904.468 + 0.14335d*E [10098]. Elements given in the gam UMi |Table represent observations in 1964 - 1968. According to gam UMi |[09906] Vr var in 1922 with P = 0.108449d. eps UMi |VB A (B 12.5m, 76.9", 3deg). Min II 4.21. S Vel |Min II 7.83; d = 0.041P. P var? There is a non-linear term S Vel |in the elements given in the Table: +4.47d*10**(-9)*E**2. W Vel |P var. Max = 2415053 + 384.3d*E (JD2414600 - 17400); W Vel |Max = 2426080 + 399.9d*E (JD2422400 - 27300); W Vel |Max = 2429990 + 388.0d*E (JD2427300 - 30100); W Vel |Max = 2438328 + 398.7d*E (JD2430100 - 38800); W Vel |since JD2438800 - see Table. OH emission. Y Vel |P var. Max = 2415900 + 438.6d*E (JD2411500 - 15900); Y Vel |Max = 2419930 + 447.7d*E (JD2415900 - 19930); Y Vel |Max = 2425755 + 452.8d*E (JD2421600 - 27600); Y Vel |Max = 2434150 + 439.5d*E (JD2427600 - 34200); Y Vel |since JD2434200 - see Table. Z Vel |P var. Max = 2415445 + 435.96d*E (JD2415000 - 25100); Z Vel |Max = 2425462 + 417.99d*E (JD2425100 - 29700) [00960]; Z Vel |since JD2429200 - see Table. RR Vel |Min II 10.9. RS Vel |P var. Max = 2410403 + 421d*E (JD2410400 - 16800) RS Vel |[09961]; since JD2415450 - see Table. RU Vel |VB A (B 12m sf). According to [00017], RU Vel |Max = 2414390 + 63d*E. RW Vel |P var. Max = 2413553 + 430.4d*E (JD2413500 - 18500); RW Vel |Max = 2420610 + 465.7d*E (JD2418500 - 25700); since RW Vel |JD2425700 - see Table. RX Vel |Min II 10.5. RY Vel |[A/H] = -0.3. P var. Max = 2440246.67 + 28.1270d*E RY Vel |(JD2419000 - 40250) [05366]; since JD2443900 - see Table. SW Vel |P var. Max = 2434872.95 + 23.473d*E - 3.75d*10**(-5)*E**2 SW Vel |(JD2412500 - 35500) [09636]. Since JD2440700 - see Table. SX Vel |The light curve has double maximum. The epoch of SX Vel |the primary (second) maximum is given in the Table. TT Vel |Min II 10.7. UW Vel |In the region of the open cluster NGC 3033. YZ Vel |Min II 12.8; DII = 0.040P; Min II - Min I = 0.537P. ZZ Vel |Min II 10.0. AA Vel |Min II 9.9. AC Vel |Min II 9.11. AF Vel |(k - b)2 = 0.06. Blazhko effect is possible [10110]. AH Vel |SB? [10111]. In the region of the open cluster AH Vel |Collinder 173. AI Vel |Mu = 0.11", P = 76deg; (k - b)2 = 0.23. AI Vel |Light oscillations with the period P0 given in the Table AI Vel |are superimposed by oscillations with P1 = 0.08620868d and AI Vel |twice smaller amplitude. According to [10112] P0 is AI Vel |constant, P1 is increasing. AK Vel |In the region of the open cluster Collinder 173. AL Vel |d = 0.072P. AO Vel |In the region of the open cluster Collinder 173. AO Vel |Min II 9.55:. There is apsidal line motion. AO Vel |There is a sinusoidal term in the elements given in the AO Vel |Table: +0.058d*sin(phi), where phi = 2pi(E - 5338)/11500, AO Vel |and E values are counted from JD2415810.66. AO Vel |Min II = 2424270.125 + 1.5845993d (E - 5338) - AO Vel |-0.058d*sin(phi); Min II - Min I = 0.792d - 0.116d*sin(phi). AP Vel |P1 = 2.19984d; P1/P0 = 0.703. M - m var (0.25P <= M - m <= AP Vel |<= 0.50P) [03710]. AQ Vel |d = 0.05P. The depth of Min II 0.05m. AS Vel |Min II 8.4; Min II - Min I = 0.55P. AT Vel |d = 0.03P. In the region of the open cluster Collinder 173. AU Vel |In the region of the open cluster Collinder 173. AV Vel |In the region of the open cluster Collinder 173. AW Vel |In the region of the open cluster Collinder 173. AX Vel |The first overtone mode light variation elements with the AX Vel |period P1 are given in the Table; the amplitude of AX Vel |the first overtone mode light variation A1 exceeds AX Vel |that of the fundamental mode, A0:A1(V) = 1.5A0(V). AX Vel |For the fundamental mode P0 Max hel = 2443878.885 + AX Vel |3.673174d*E. AX Vel |P1/P0 = 0.706; M - m var: 0.24P <= M - m <= 0.50P:. AY Vel |Min II 9.7. AZ Vel |Min II 13.0. In the region of the open cluster AZ Vel |Collinder 173. BB Vel |P < 20d. In the region of the open cluster Collinder 173. BC Vel |Min II 12.3. BD Vel |d = 0.04P. BE Vel |Min II 12.5. BF Vel |The depth of Min II 0.04m. BM Vel |Min II 13.0. In the region of the open cluster NGC 2547. BM Vel |In the region of the open cluster Collinder 173. BO Vel |Min II 14.2. BP Vel |Min II 13.7. BR Vel |The shape of the light curve varies. BT Vel |Min II 14.8. BU Vel |Min II 10.96; Min II - Min I = 0.522P. In the region BU Vel |of the open cluster Collinder 173. BV Vel |In the region of the open cluster Collinder 173. BW Vel |Min II 14.3. BX Vel |In the region of the open cluster Tr 10. BZ Vel |Min II 10.4; Min II - Min I = 0.57P. CK Vel |D ~0.3d. CL Vel |Min II 13.4. CR Vel |d = 0.05P. CS Vel |[A/H] = 0.1. Possible member of the open CS Vel |cluster Ruprecht 79. CU Vel |The period of superhumps ~0.08d, A = 0.4m [10115]. CV Vel |Min II 7.17. CW Vel |d = 0.024P. The depth of Min II 0.1m pg. CZ Vel |Min II 11.1. DF Vel |Min II 13.4. DH Vel |Min II 13.7. DK Vel |VB A (B 12.50m, 22", 315deg; C 16m, 10", 60deg). DL Vel |Min II 12.1. DM Vel |P = 123d? DQ Vel |Min II 11.0. DS Vel |Min II 10.8. DT Vel |(k - b)2 = 0.24. DX Vel |Min II 10.3. In the region of the open cluster Col 213. EH Vel |Min II 13.4. EL Vel |In the region of the open cluster Collinder 173. EO Vel |Min II 11.90, DII = 0.07P. EO Vel |Apsidal motion: Min II - Min I = 3.15d + 0.00003d*E. EO Vel |Min II = 2441716.75 + 5.32969d*E. EP Vel |In the region of the open cluster IC 2395. ES Vel |Min II 12.7. ET Vel |Min II 12.1. EU Vel |Min II 13.8. EY Vel |d = 0.04P:. FM Vel |Min II 12.9. FS Vel |Delta(S) = 10. FT Vel |Min II 10.5. FW Vel |Min II 10.0. FX Vel |Min II 10.5. The shape of the light curve varies. FY Vel |Min II 7.03. Type ELL? [06827]. FZ Vel |VB A (B 12.08m, 24.2", 338deg). GG Vel |VB A (B 11.2m, 6", delta(alpha) = 0). P = 2.950432d? GP Vel |<Min II> 6.90. Min II - Min I = 0.55P. GP Vel |The shape of the light curve varies. GP Vel |There are probably long-period light GP Vel |oscillations: Min = 2442681.6 + 93.3d*E (A ~0.02m) GP Vel |[10051]. The period of X-ray pulses var: 282.8913s GP Vel |(1975.5) [10125]; 282.919s (1975.7) [10126]; 282.869s GP Vel |(1976.4), 282.838s (1976.9) [10127]; 282.80s (1978.9) GP Vel |[10128]; 282.745s (1979.3), 282.7874s (1980.3), 282.87s GP Vel |(1981.0) [10129]; 282.93s (1981.9 - 1982.9); 282.9306s GP Vel |(1983.2) [10078]. GV Vel |In the region of the open cluster NGC 2660. HU Vel |Pulsar PSR 0833-45. In the nebula Vela SNR. HU Vel |Star M [08276]. The pulsed radiation varies in radio, HU Vel |optical and gamma rays with P = 0.089s. HU Vel |P var [10136 - 10139]: P = 0.089233318274s HU Vel |(JD2442553 - 680), P = 0.089234713929s (JD2442700 - 848), HU Vel |P = 0.089244007685s (JD2443654 - 676), P = 0.089245406487s HU Vel |(JD2443719 - 850) [10137]; P = 0.089256985348s HU Vel |(JD2444795.84) [10138]. HV Vel |A member of the open cluster IC 2391. HW Vel |P = 0.26133d? A member of the open cluster IC 2391. HX Vel |VB A (B 7.1m, 0.3", 313deg, 1949); in the region HX Vel |of the open cluster IC 2395. Min II 5.50:. HY Vel |VB A (B 5.7m, 76.6"); a member of the open cluster IC 2391. HY Vel |Min II 4.90. IL Vel |A var (0.02m <= A <= 0.15m). Beat period 10.075d IL Vel |(Min A = 2443175.5 + 10.075d*E). IM Vel |VB A (B 9.73m, 3.3", 179deg, 1948). IM Vel |The double wave of light variations IM Vel |with rotation period Prot = 2.85204d and A = 0.03m is IM Vel |superimposed by oscillations with the periods IM Vel |P1 = 0.00812815d (A1 = 0.0043m), P2 = 0.00808206d IM Vel |(A2 = 0.0035m), P3 = 0.00810503d (A3 = 0.0008m), P4 = IM Vel |0.004052519d (A4 = 0.0009m), P5 = 0.004064065d IM Vel |(A5 = 0.0004m), P6 = 0.004041031d (A6 = 0.0004m), IM Vel |P7 = 0.00815128d (A7 = 0.0004m) [09208]. IN Vel |P = 65 - 70d, IP Vel |VB A (B 11.2m V, 2.1", 200deg, 1929). P > 1.25d. IQ Vel |Min II 12.94; Min II - Min I = 0.500P. IS Vel |A(U) var: 0.005m <= A(U) <= 0.018m. IT Vel |Min II 7.08. P = 23.52d? OQ Vel |The type is doubtful. V0360 Vel |Several close companions. gam 2 Vel |VB A (B 4.22m, 41.3", 220deg). gam 2 Vel |SB2 (Porb = 78.5002d [10119]). In HII region. gam 2 Vel |T0 = 2433633.0 is the epoch of the conjunction where the gam 2 Vel |O component is in front [10119]. lam Vel |VB A (B 14.8m, 18.2", 137deg). omi Vel |A member of the open cluster IC 2391. P(VR) = 2.74d. omi Vel |P = 2.76d? SB1? The epoch of the light maximum is given. omi Vel |Close binary system? R Vir |P var. Max = 2381914 + 145.77d*E (JD2338900 - 2402000); R Vir |Max = 2402321 + 144.90d*E (JD2402000 - 18000); R Vir |Max = 2418268 + 145.48d*E (JD2418000 - 30000); R Vir |Max = 2430489 + 148.32d*E (JD2430000 - 34000); R Vir |Max = 2434193 + 144.63d*E (JD2434000 - 38500); R Vir |Max = 2438829 + 147.45d*E (JD2438500 - 43000); R Vir |since JD2443000 see Table. Maser (SiO). S Vir |P var. Max = 2399014 + 374.7d*E (JD2398600 - 2405000); S Vir |Max = 2412970 + 376.2d*E (JD2412000 - 23500, on average); S Vir |Max = 2423502 + 381.52d*E (JD2423500 - 23000); since S Vir |JD2433000 - see Table. Maser (H2O, SiO). T Vir |Maser (OH, H2O, SiO). V Vir |P var. Before JD2427000 Max = 2400467 + 250.17d*E; V Vir |Max = 2427225 + 246.54d*E (JD2427000 - 31500); V Vir |since JD2431500 - see Table. W Vir |The epoch of Min is given. P var. W Vir |Min = 2404151.168 + 17.2707d*E (JD2403000 - 23200); W Vir |Min = 2423200.837 + 17.2634d*E (JD2423200 - 29700); W Vir |since JD2429700 - see Table. The light curve shape var. W Vir |[Fe/H] = -1.03. X Vir |VB A (B 12m, dK4, 0.6', ~50deg). The brightenings X Vir |of 1871 and 1882 may be due to misidentification [01651]. Z Vir |mu alpha = +0.0098S, mu delta = -0.120". Z Vir |P var. Max = 2409683 + 309.19d*E (JD2408000 - 18500); Z Vir |since JD2418500 - see Table. RS Vir |Maser (OH, H2O, SiO). P var. Max =2412592 + 351.29d*E RS Vir |(JD2412000 - 31000); since JD2431000 - see Table. RT Vir |Maser (OH, H2O, SiO). According to [10145], observations RT Vir |of 1970-1977 are not in agreement with the P value in the RT Vir |Table. RU Vir |P var? Max = 2425120 + 435.9d*E (JD2414000 - 31500); since RU Vir |JD2431500 - see Table. RV Vir |P var. Max = 2412272 + 268.39d*E (JD2412000 - 31500); RV Vir |since JD2431500 - see Table. RX Vir |VB (B 13.0m vis, 1.1", 107deg, 1939). According to RX Vir |photoelectric observations [06450,08837], 8.72m - 8.81m V. RX Vir |Const? [06450]. SS Vir |P var. Max = 2415910 + 352.75d*E (JD2415900 - 21500); SS Vir |Max = 2421913 + 361.7d*E (JD2421500 - 26500); SS Vir |Max = 2428359 + 350.12d*E (JD2426500 - 40000); SS Vir |since JD2440000 - see Table. ST Vir |P var. Max = 2425005533 + 0.4108494d*E (JD2422000 - 29100) ST Vir |[10146]; Max = 2436702.513 + 0.4108168d*E ST Vir |(JD2433000 - 39000) [03415]; since JD2439000 - see Table. ST Vir |Blazhko effect? Delta(S) = 0.8. SU Vir |P var. Max = 2415040 + 213.7d*E (JD2415000 - 19500); SU Vir |Max = 2419926 + 210.96d*E (JD2415000 - 31500); SU Vir |Max = 2437378 + 210.2d*E (JD2431500 - 38500); SU Vir |since JD2438500 - see Table. SV Vir |P var? The mean elements are given. Maser (H2O). SZ Vir |Possibly EW with a very small A. TV Vir |VB A (B P). TW Vir |Porb = 0.182666d [09430]. Variability of ellipsoidal TW Vir |character in H light: P = Porb/2, A(H) = 0.13m. TW Vir |X-ray source. TX Vir |VB A (B 15m, 0.3' P). TY Vir |[Fe/H] = -1.7. TZ Vir |P2 = 6900d is superimposed? UU Vir |[Fe/H] = -0.3. delta[S] = 0.7. UW Vir |d = 0.011P. P var. Min = 2419942.513 + 1.8106818d*E UW Vir |(JD2415000 - 34500); since JD2441000 - see Table UY Vir |d = 0.014P; Min II 8.1. VV Vir |Min II 12.2:. VW Vir |SN 1895 (NGC 4424). XX Vir |[Fe/H] = -1.5. Delta(S) = 9:. YZ Vir |[A/H] = -0.9. AD Vir |P var. Max = 2425259.259 + 0.5522109d*E AD Vir |(JD2419000 - 31000); since JD2431000 - see Table. AF Vir |P var. Max = 2429051.697 + 0.4838214d*E AF Vir |(JD2419500 - 36000); Max = 2436718.3758 + AF Vir |0.4838386d*E (JD2436000 - 37500) [10159]; AF Vir |since JD2440000 - see Table. DM var. AG Vir |The depth of Min II up to 0.44m. AG Vir |The light curve shape and A var. AG Vir |dI = 0.03P:, dII = 0.66P. Min II - Min I = 0.512P. AG Vir |P var. Min = 2434487.4297 + 0.6426489d*E AG Vir |(JD2424500 - 34500); since JD2434500 - see Table. AH Vir |mu alpha = +0.0015S, mu delta = -0.111" AH Vir |ADS 8472 A (B 13.2m, 1.3", 17deg). AH Vir |The combined brightness is given, AH Vir |dI = 0.07P. The depth of Min II 0.53m, dII = 0.00P. AH Vir |The light curve shape var. AH Vir |P var. Min = 2434841.3963 + 0.40751843d*E AH Vir |(JD2425000 - 35000) [05222]; Min = 2435573.710 + AH Vir |0.40752192d*E (JD2435000 - 41400); Min = AH Vir |2441411.460 + 0.40753186d*E (JD2441400 - 44000); AH Vir |since JD2444000 - see Table. AK Vir |VB B (A = BD -17deg 3996; B 44", 286deg). AL Vir |P var [A/H] = -0.7. AN Vir |P2 ~1000d is superimposed. AO Vir |VB A (B 11.4m vis, 6.9", 321deg, 1956, common AO Vir |Vr). delta(M) is possibly in error because of the AO Vir |companion. P var. Max = 2413949 + 256.88d*E AO Vir |(JD2412900 - 21000); since JD2421000 - see Table. AS Vir |P var. The Table gives the mean elements valid after AS Vir |JD2425600. Blazhko effect? [03506]. AS Vir |(k - b)2 = 0.08. AT Vir |P var. Max = 2426831.367 + 0.5258053d*E AT Vir |(JD2420500 - 35000) [00188]; since JD2435000 - see Table. AT Vir |(k - b)2 = 0.00, Delta(S) = 6.0. AU Vir |[Fe/H] = -1.84, Delta(S) = 10.1. AV Vir |Delta(S) = 5.5. AW Vir |Min II 11.67. AX Vir |Min II 10.24. AY Vir |Maser (H2O). AZ Vir |Min II 11.37. BB Vir |Blazhko effect? BC Vir |P var. Max = 2419922.289 + 0.56451468d*E BC Vir |(JD2419900 - 30100); the Table gives current elements. BD Vir |P var. Min = 2424971.720 + 2.548410d*E BD Vir |(JD2424900 - 32000); since JD2432000 - see Table. BF Vir |Min II 10.72. Total eclipses. BF Vir |P var. Min = 2416595.67 + 0.64057d:*E (JD2414000 - 19000); BF Vir |Min = 2440331.809 + 0.64057631d*E BF Vir |(JD2426000 - 41000); since JD2441000 - see Table. BH Vir |Min II 10.24. Distortion wave? BH Vir |(Delta(V) = 0.04m). BN Vir |P var. Max = 2419865.422 + 0.39127585d*E BN Vir |(JD2419800 - 28300); since JD2432600 - see Table. BO Vir |P var. Max = 2419513.388 + 0.52005916d*E BO Vir |(JD2419500 - 33000); since JD2433000 - see Table. BQ Vir |P var? BS Vir |[Fe/H] = -1.84. Delta(S) = 10.1. BV Vir |P var. Max = 2426070.488 + 0.4965803d*E BV Vir |(JD2419900 - 28500); since JD2436600 - see Table. BW Vir |P var. Max = 2420247.403 + 0.4706660d*E BW Vir |(JD2420200 - 26800); since JD2426800 - see Table. CG Vir |Min II 10.9. CK Vir |[Fe/H] = -2.0. CM Vir |d = 0.05P. P var. Min = 2425411.330 + 3.40167d*E CM Vir |(JD2423900 - 28400) [00001]; during JD2432200 - 34200 - see CM Vir |Table. CS Vir |The epoch of Max in B light is given. CS Vir |SB (Porb = 1618d). IR excess (4.8 mkm). CU Vir |ADS 9152 A (B 11.9m, G1V, 60", 212deg). CW Vir |The epoch of min is given. CX Vir |The depth of Min II 0.30m. DK Vir |According to [10189], P1 = 0.1162d, P2 = 0.1086d. DK Vir |(k - b)2 = 0.20. DL Vir |SB (Porb = 2286d). DL Vir |The spectrum shows the A-component of the eclipsing DL Vir |system and the G8III star around which the eclipsing DL Vir |system is orbiting. DM Vir |Min II 9.49. DII = DI. DN Vir |P >= 100d. DT Vir |Mu alpha = -0.044s, mu delta = -0.02". SB? DT Vir |Rotation period 1.535d [10014], A = 0.05m V. DV Vir |Blazhko effect? EF Vir |According to [04784], const?, 16.1m pg. EP Vir |IR excess (4.8 mkm). EQ Vir |SB; [Fe/H] = -0.08; mu alpha = -0.018s, mu delta = -0.09". EQ Vir |Min = 2441129.585 + 3.914169D*E + 0.0001803345d*E**2, EQ Vir |A = 0.10m V, M - m = 0.40P. Soft X-ray source, EQ Vir |lg FX/FV = -2.07. EW Vir |P >= 100d. EX Vir |P >= 100d. EY Vir |P >= 100d. FF Vir |The P value for magnetic field variations is given. FG Vir |ADS 8471 A (B 13.51m, 25", 352deg, 1909; FG Vir |C 11.85m, 74", 195deg, 1909). FI Vir |Mu alpha = +0.043s, mu delta = -1.22". FL Vir |VB AB (A = 0.76", P = 16A). Both components show flares? FL Vir |The range of combined brightness is given. FL Vir |Mu alpha = -0.118s, mu delta = +0.26". FM Vir |SB2, Porb = 38.324d. FN Vir |Mu alpha = -0.064s, mu delta = +0.28". SB? FN Vir |X-ray source, LX/Lbol = -3.55. FO Vir |Min II 6.67. FQ Vir |Deep Min II. GG Vir |Multiperiodicity, 0.023d <= P <= 0.083d, A <= 0.02m. GH Vir |P var. GK Vir |The secondary is a red dwarf (M0 - M6). GL Vir |Mu alpha = -0.087s; mu delta = +0.23". GM Vir |P ~1.6d/n. GQ Vir |Mu alpha = -0.045s, mu delta = -0.44". GR Vir |The depth of Min II 0.41m. GU Vir |P var. Max = 2439236.36 + 0.466562d*E GU Vir |(JD2438100 - 39300); during JD2441300 - 42600 - see Table. LV Vir |Type RR: is also possible. MW Vir |Type DSCTC: is also possible. NN Vir |Type EW: is also possible. alf Vir |The Table gives the epoch of Min for the ellipsoidal alf Vir |variability and Porb. The depth of Min II up to 0.08m. alf Vir |SB 2. e = 0.205 +- 0.004. Apsidal motion: Pi = 108a +- 5a. alf Vir |Pulsations: P var, P = 0.17378587d (1908 - 1956); alf Vir |since 1956 Max = 2445405.63 + 0.17378680d*E [10181]. A var. alf Vir |3 companions according to lunar occultation observations: alf Vir |3.1m, 0.0025"; 4.5m, 0.05"; 7.5m, 0.5". Soft X-ray source, alf Vir |LX/Lbol = 2.9*10**(-8). psi Vir |Binary? (lunar occultations). R Vol |P var. Max = 2415238 + 441d*E (JD2394100 - 2418800) R Vol |[10143]; since JD2422700 - see Table. S Vol |P var. Max = 2415042 + 397.6d*E (JD2415000 - 24200), S Vol |Max = 2428880 + 392.1d*E (JD2423000 - 28900), S Vol |Max = 2434113 + 401.7d*E (JD2428900 - 34900), S Vol |Max = 2434910 + 387.2d*E (JD2434900 - 39200); S Vol |since JD2439200 - see Table. T Vol |P var. Max = 2413135 + 189.8d*E (JD2413100 - 14600); T Vol |Max = 2416870 + 171.8d*E (JD2414600 - 16900); T Vol |Max = 2416870 + 176.8d*E (JD2416800 - 24400); T Vol |Max = 2424460 + 170.8d*E (JD2424400 - 27200); T Vol |Max = 2429925 + 182.3d*E (JD2427200 - 30000); T Vol |since JD2440000 see Table. RX Vol |P < 20d? ST Vol |SP component of a very close pair. SV Vol |The shape of the light curve varies. TX Vol |Min II 10.5. P var. Min I = 2416789.869 + 5.38845d*E TX Vol |(JD2415100 - 26000), Min I = 2431150.345 + TX Vol |5.3887d*E (JD2426000 - 31400), Min I = TX Vol |2433542.609 + 5.388d*E (JD2431400 - 33600) TX Vol |[00001]; since JD2433600 see Table. R Vul |P var. Max = 2400169 + 138.3d*E (JD2400100 - 02700), R Vul |Max = 2402779 + 136.76d*E (JD2402700 - 19800), R Vul |Max = 2419880 + 137.45d*E (JD2419800 - 24400), R Vul |Max = 2424413 + 136.76d*E (JD2424400 - 28500 R Vul |[00960]; Max = 2429331 + 135.9d*E (JD2428500 - 32000) R Vul |[00001]; since JD2432000 see Table. S Vul |In the region of the open cluster C 1947 + 272 [10123]. S Vul |P var. Max = 2401772 + 67.37d*E (JD2401760 - 6400), S Vul |Max = 2408180 + 67.70d*E (JD2408170 - 14950), S Vul |Max = 2415285 + 68.26d*E (JD2415300 - 22800), S Vul |Max = 2423468 + 67.72d*E (JD2423450 - 27200), S Vul |Max = 2428227 + 68.18d*E (JD2428220 - 31300) S Vul |[00761]; Max = 2432775 + 67.51d*E (JD2431300 - 34500) S Vul |[10148]; Max = 2437150 + 68.66d*E S Vul |(JD2436800 - 39600), Max = 2441507 + 67.344d*E S Vul |(JD2439600 - 43000) [10124]; since JD2443000 see Table. S Vul |[A/H] = 0.1. T Vul |P var. Max = 2419372.151 + 4.435589d*E (JD2409880 - 34000); T Vul |since JD2434000 see Table. V Vul |Min II 8.65. P var. Min I = 2414912.9 + 74.96d*E V Vul |(JD2414900 - 20840), Min I = 2420909.8 + 75.686d*E V Vul |(JD2420900 - 24810), Min I = 2425072.9 + 76.344d*E V Vul |(JD2425050 - 30000), Min I = 2430023.5 + 75.957d*E V Vul |(JD2430000 - 32500) [10149]. Study of period variation and V Vul |changes of Min II by Min I see also in [00767,010150]. W Vul |In the region of the open clusters NGC 6882, NGC 6885. X Vul |P var. Max = 2420636.337 + 6.319301d*E (JD2417000 - 34000) X Vul |[00768]; since JD2435000 - see Table. Z Vul |VB A (B 12.0m, 13", 359deg). Min II 7.58. P var. Min I = Z Vul |2425456.117 + 2.454926d*E (JD2413200 - 37000) Z Vul |[00063]; since JD2437000 - see Table. RS Vul |Min II 6.86; Min II - Min I = 0.508P. RU Vul |A var. P var. Max = 2416266 + 155.95d*E RU Vul |(JD2415000 - 36000), Max = 2436779 + 150.7d*E RU Vul |(JD2436000 - 38800), Max = 2438855 + 153.4d*E RU Vul |(JD2438800 - 41620), Max = 2441193 + 138.5d*E RU Vul |(JD2441620 - 42600); since JD2442600 - see Table. RX Vul |P var. Max = 2420301 + 438d*E (JD2418900 - 22500) RX Vul |[04018]; since JD2424700 - see Table. RZ Vul |Slow variations of mean brightness with P = 1410D and RZ Vul |A = 2m are superimposed by fluctuations with the cycle RZ Vul |40 - 100d and A up to 1m. SU Vul |In the region of the open cluster NGC 6882, NGC 6885. SV Vul |[Fe/H] = 0.23. P var. There is a nonlinear term in the SV Vul |elements given in the Table: -0.0001814d*E**2. SX Vul |In the region of the open cluster NGC 6940. UU Vul |The co-ordinates are wrong? UU Vul |[10156]. VV Vul |Min II 12.1; d = 0.026P. P var. Min I = 2416670.527 + VV Vul |3.411224d*E (JD2416600 - 27500) [00134]; VV Vul |since JD2426000 - see Table. VW Vul |Porb = 0.0731d [10160]. VY Vul |Min II 14.4:. WW Vul |There is quasi-periodicity in light minima with the cycle WW Vul |404d. XZ Vul |Min II 11.4. P var. Min I = 2426477.525 + 3.0895116d*E XZ Vul |(JD2416900 - 36000) [04427]; since JD2436000 - see Table. AB Vul |The depth of Min II 0.02m. AD Vul |Min II 0.010P. AF Vul |Min = 2436545.23 + 0.954d*E (JD2436200 - 900) [03148]. AR Vul |In the region of the open cluster Stock 1. AT Vul |Min II 9.3; d = 0.02P. AW Vul |Min II 10.9; d = 0.020P. AX Vul |d = 0.018P. AY Vul |d = 0.020P. P var. Min hel = 2436128.388 + 2.4124239d*E AY Vul |(JD2418500 - 40700); since JD2440700 - see Table. AZ Vul |Min II 11.9. BB Vul |In the region of the open cluster NGC 6940. BE Vul |VB A (BC 11.92m, 50", 320deg). Min II 9.90. P var. BE Vul |Min I = 2426144.490 + 1.55205d*E BE Vul |(JD2426140 - 28880), Min I = 2430698.203 + BE Vul |1.5520442d*E (JD2430690 - 34660), Min I = BE Vul |2435340.373 + 1.552052d*E (JD2435340 - 40070); BE Vul |since JD2440100 - see Table. BF Vul |Elements given in the Table represent well only the bright BF Vul |maxima. The fainter maxima are represented by the elements: BF Vul |Max = 2427731 + 95.4d*E. BI Vul |Min II 14.86. P var? Min I = 2424759.70 + 0.251828d*E BI Vul |[00193]; since JD2444750 - see Table. BN Vul |Delta(S) = 7. P var. Max = 2414815.759 + 0.5941295d*E BN Vul |(JD2414000 - 30000) [00388]; Max = 2434244.333 + BN Vul |0.59412538d*E (JD2430000 - 36000) [00616]; BN Vul |Max = 2438265.386 + 0.59412763d*E (JD2436000 - BN Vul |41000) [09009]; since JD2441000 - see Table. BO Vul |Min II 10.6. P var. Min I = 2429984.332 + 1.9459123d*E BO Vul |(JD2415000 - 30000) [00007]; Min I = 2432379.766 + BO Vul |1.9459206d*E (JD2427000 - 35000), since BO Vul |JD2435300 - see Table. BP Vul |Min II 10.5. BS Vul |Min II 11.10. BT Vul |d = 0.03P; Min II 12.3. BU Vul |P var. Min = 2431006.204 + 0.5689904d*E BU Vul |(JD2426500 - 31100) [00001]; since JD2433500 - see Table. BV Vul |S 6.5/6-. BW Vul |P var. Max = 2424000.171 + 0.20102229d*E BW Vul |(JD2424000 - 26500), Max = 2426500.079 + BW Vul | + 0.20102933d*E (JD2426500 - 31500), Max = BW Vul |= 2432000.054 + 0.20103513d*E (JD2431500 - 41000); BW Vul |since JD2441000 - see Table. CD Vul |Min II 11.9. CK Vul |Max 2331186:. Connected with nebulae. Type NR? CS Vul |Min II 13.6. DR Vul |Min II 9.19; DII = 0.132P. DR Vul |There is apsidal motion with the period 37.8 years. DR Vul |Elements given in the Table contain supplementary DR Vul |terms: -0.07165d*sin(0.05863deg*E) - 0.00269d* DR Vul |*sin(0.11726deg*E). DR Vul |Min II = 2440301.7934 + 2.2508645d*E + 0.07165d* DR Vul |*sin(0.05863deg*E) - 0.00269d*sin(0.11726deg*E). DR Vul |P var? [10185]. The depth of minima varies. DY Vul |VB A (B 13.0m V, 14", 300deg). EH Vul |P var. Max = 2429609 + 185d*E (JD2429600 - 30600); EH Vul |since JD2430800 - see Table. EP Vul |S 6.5/5. EQ Vul |Min II 12.5; Min II - Min I = 0.31P; DII = 0.050P, EQ Vul |dII = 0.010P. ER Vul |P var. Min I = 2440182.2593 + 0.69809510d*E ER Vul |(JD2433100 - 40200) [08592]; since JD2440100 - see Table. ER Vul |7.35m <= Min II <= 7.44m. The shape of the light ER Vul |curve and depths of minima vary. ES Vul |VB A (B 10.1m, 1.6", 126deg). ET Vul |[A/H] = -0.4. P var. Max = 2425110.63 + 54.33d*E ET Vul |(JD2422900 - 26600), Max = 2432875.80 + 54.33132d*E ET Vul |(JD2432700 - 35430), Max = 2438656.99 + 53.81d*E ET Vul |(JD2436050 - 39035), Max = 2439253.55 + 54.24d*E ET Vul |(JD2439035 - 40990) [10168]; since JD2441900 - see Table. EU Vul |Min II 13.3. EV Vul |Min II 11.9. P var. Min I = 2428750.459 + 2.822084d*E EV Vul |(JD2428400 - 36400) [04027]; Min I = 2436748.37 + EV Vul |2.82220d*E (JD2436380 - 750) [03732]; since EV Vul |JD2441500 - see Table. EX Vul |d = 0.03P. EY Vul |The depth of Min II 0.05m. FG Vul |In the region of the open cluster NGC 6940. Star 120. FG Vul |The epoch of light minimum is given. FH Vul |P var. The elements given in the Table are valid since FH Vul |JD2436000. FK Vul |Blazhko effect. FM Vul |Min II 13.0. FN Vul |d = 0.02P; Min II 14.2. FP Vul |Min II 15.6. FQ Vul |Min II 12.9. Apsidal motion with P = 280 years. Correction FQ Vul |of mispints in [04248] see in [04244]. FR Vul |Probably the period must be doubled. FS Vul |Min II 15.2. FU Vul |sp component of a close pair. FW Vul |Min II 12.9. FY Vul |sp component of a close pair. Cycle 30 - 70d [04027]. FZ Vul |Min II 13.9. GG Vul |P var. Max = 2427681.0 + 106.5d*E (JD2427500 - 28850); GG Vul |since JD2428850 - see Table. GH Vul |P = 2.5d? GI Vul |Min II 13.8. GK Vul |Red. GN Vul |Min II 12.4; d = 0.04P. GO Vul |Min II - Min I = 0.515P. The depth of Min II 0.03m. GP Vul |Min II 11.2; Min II - Min I = 0.48P. GQ Vul |nf component of a close triple group of stars. GQ Vul |P var. Max = 2434399.825 + 12.647241d*E (JD2426100 - 38000) GQ Vul |[04414]; since JD2444600 - see Table. GR Vul |Min II 13.3. The chart in [04244] is wrong. GT Vul |Min II 15.8. GU Vul |Min II 12.2. GV Vul |Probably the period must be doubled. Probably the period GV Vul |must be doubled. HI Vul |Min II 12.6. HP Vul |The depth of Min II 0.04m. HS Vul |Min II 14.2. HU Vul |Blazhko effect? HV Vul |P var. Max = 2437165.449 + 0.419906d*E (JD2437100 - 38670); HV Vul |since JD2438670 - see Table. Blazhko effect? HW Vul |P var. Max = 2429077.0 + 75.44d*E (JD2427190 - 29080), HW Vul |Max = 2429077.0 + 73.94d*E (JD2429070 - 32470); HW Vul |since JD2432350 - see Table. IU Vul |P var. Max = 2434656 + 320.2d*E (JD2432700 - 37860) [04427]; IU Vul |since JD2437860 - see Table. IW Vul |Min II 13.1. KN Vul |Min II 13.4. KO Vul |Red. KS Vul |Very red. LT Vul |Multiperiodicity: P1 = 0.109414d, A1(V) = 0.0234m; LT Vul |P2 = 0.11094d, A2(V) = 0.0074m; P3 = 0.1215d, LT Vul |A3(V) = 0.0070m (JD2444054 - 096) [10173]; LT Vul |P1 = 0.109621d, A1(B) = 0.0340m; P2 = 0.093528d, LT Vul |A2(B) = 0.0136m (JD2444071 - 465) [10193]. LU Vul |Nova Vul 1968 N2. LV Vul |Nova Vul 1968 N1. VB A (B 18m, 6", 115deg). LW Vul |Min II 16.3. MN Vul |Min II 16.1; Min II - Min I = 0.518P; DII = 0.10P. MO Vul |Min II 14.8. P var? MR Vul |P2 = 111.0d? MT Vul |Multiperiodicity: MT Vul |P2 = 119.93d (A2 = 0.3m), P3 = 25.02d (A3 = 0.4m:). MX Vul |P = 181.8d? NO Vul |Min II 14.1. NS Vul |VB A (B 8.8m, A0, 0.73", 273deg, 1978.6), NS Vul |The range of combined light variation is given. PS Vul |VB A (B 10.0m, 0.4", 105deg, 1980.0); SB2. PT Vul |P1 = 256.12714s (A1 = 1.14%), Max1 = PT Vul |2445166.660914 HJED; P2 = 256.33205s (A2 = 1.09%), PT Vul |Max2 = 2445166.659424 HJED; P3 = 128.11496s (A3 = 0.37%), PT Vul |Max3 = 2445166.660024 HJED. mu = 0.1508", P=1.6deg. PU Vul |Pre-outburst SP M4 (1958). Gradual light increase in PU Vul |1977 - 79 up to 8.7m V; in 1979 A = 0.29M V, PU Vul |Min I = 2443943.39 + 78.12d*E [10197]. In the max of 1979 PU Vul |Sp F5Ia - F8-9I. In February 1980 an abrupt light decrease PU Vul |started; the star reached V = 13.65m by early September. PU Vul |By September, 1981 the star recovered from the deep Min of PU Vul |500d duration. During the 1980 - 81 minimum Sp M5 with TiO PU Vul |bands, emissions of Halpha, NaD, [OII], FeII, rare earths. PU Vul |In 1982 - 84 8.35m - 8.87m V, Sp became F again. Simetimes PU Vul |Halpha, Hbeta emissions have been detected, often PU Vul |with P Cyg profiles. V0398 Vul |Not identical to IRC+30416 = NSV 12861. --------------------------------------------------------------------------------------------