WD0000-014 See also (RF)(RS)
WD0000-345 See also (OJ)
WD0001+433 See also (QM)(RK)
WD0002+165 See also (PP)
WD0003-570 WD0003-570 consists of a non-magnetic WD and a late-type cool dwarf. (GU)
WD0004+330 See also (QP)(QM)(NB)(NL)(RK)
WD0005+511 Similar to the PG1159 degenerates but fewer, weaker metals and Balmer emission,X-ray corona,mass loss, Ref.(60)(84)(SM).
WD0005-163 Temperatures ambigious. Ref.(PP)
WD0005-267 PCEB. Ref.(QH).
WD0008+424 See also (PV)(OJ)
WD0009+501 WD0009+501 is a magnetic degenerate,the first known below 100 kilogauss, Ref.(9W)(9V) See also (PV)(OL)(OJ)(MV)(NB)(RQ)
WD0010-000 See also (NC)
WD0011-134 LHS1044 is a magnetic degenerate, Ref.(31) See also (PV)(MV)(NN)(OJ)
WD0012+008 See also (OY)
WD0013+008.1 See also (NC)
WD0014+003 See also (QJ)(NC)
WD0014-006 See also (QJ)(NC)
WD0014-015 See also (MS)(NR)
WD0015+004 See also (MV)
WD0015-004 See also (PJ)(NC)
WD0016+000 See also (QJ)
WD0016-220 See also (PP)
WD0016-258 Long period ZZ Ceti (OC)
WD0018+147 See also (PD)(MV)
WD0018-267 See also (OL)
WD0019-105 Double-degenerate merger system. Ref.(QT).
WD0019-113 See also (QJ)
WD0019-287 ZZ Ceti candidate (HC)
WD0022+274 See Also (PR)
WD0022-400 CPMB with APMPN 0025-3949A as second component (IN).
WD0023+144 See also (NC)
WD0023+388 Triple star system, also identifies G171-B10B as the WD and G171-B10A as the MS. Ref.(MK) Likely closer to d~60pc Ref.(MQ) See also (QR)(QP)
WD0023-109 Mis-identified as WD0023+109 in REf.(NZ) CPMB system with the K-star G158-077. Ref.(OF) Likely triple system - DA+dM0(G158-78B)+DC8(G158-78C). Ref.(PS)
WD0024-010 See also (NC)
WD0024-556 See also (PP)
WD0025+000 See also (QJ)(NC)
WD0025-004 See also (QJ)(NC)
WD0025-277 ZZ Ceti candidate (HC)
WD0027+151 See also (RS)
WD0027-549 See Also (PR)
WD0027-636 See also (QM)(PP)(JV)(RK)
WD0028-274 See section A1.2 in Ref. (LJ).
WD0028-474 Double-lined double-degenerate binary. Ref.(PP)
WD0029+571 PG1159-like central star of SH2-136.(66).
WD0029-181 See also (PP)
WD0030+006 See also (NC)
WD0030+444 Binary (DA5+G8) system. Ref.(MK)
WD0030-001 See also (NC)
WD0031-311 See also (PP)
WD0032-175 See also (MR)(OH)
WD0033+016 See also (PP)(MY)
WD0033-007 See also (NC)
WD0034+002 See also (PY)
WD0034+008 See also (NC)
WD0034-211 Close double degenerate binary, Ref.(45),(MQ) MS companion= LTT 0329B See also (MY)
WD0036+312 Short period ZZ Ceti (OC)
WD0037+312 See also (JV)(NL)
WD0037-006 Double-lined double-degenerate binary. Ref.(PP) See also (OK)
WD0038+555 G218-008 has strong UV absorption features, Ref.(CG).
WD0038-226 LHS 1126 is the only know white dwarf to show JHK absorption, strong C2? H2? opacity, Ref.(DQ)(5X) See also (PV)(OL)(OJ)(MM)
WD0039+149 See also (NC)
WD0040+000 See also (PD)
WD0041+092 Hot DA companion to the rapidly rotating K1-3V star BD+08 102, REF.(82)(4D).
WD0041-102 FEIGE 7 is a magnetic white dwarf, Ref.(5F)(03).
WD0044-121 NGC246 is a PG1159 star with several detected periods and an associated planetary nebula; type lgE, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
WD0045+000 See also (NC)
WD0046+051 VAN MAANEN2 was the only example of a DG white dwarf, Ref.(DB) See also (PV)(2L)(NN)(OE)(OJ)
WD0047+190 See also (QV)(MR)
WD0047-524 See also (PP)(NL)
WD0048-202 Possible sdOB/WD binary system. Ref.(QX).
WD0048-294 See also (JV)
WD0048-544 See also (PP)
WD0049-011 See also (NC)
WD0050-011 Post-common envelope binary. Ref.(QB)See also (QJ)(NC)(QH)
WD0050-332 See also (PP)(JV)(MV)(NB)(NL)(RK)
WD0051+006 See also (QJ)
WD0052+004 See also (NC)
WD0052-006 See also (QJ)(PE)(NC)
WD0052-101 See also (OK)
WD0053-103 See also (NC)
WD0054-004 Reclassified as M star; Ref.(QB)
WD0055+006 MS+MS superposition; Ref.(QB)
WD0057+003 See also (NC)
WD0058+148 See also (QJ)(NC)
WD0058-044 See also (PP)
WD0059-008 ZZ Ceti star Ref.(KB)
WD0101+002 See also (QJ)(NC)
WD0101+003 See also (QJ)(NC)
WD0101+048 Double degenerate system. Ref.(JP)See also (PP)(OJ)(MM)(NB)(NL)(OL)
WD0101+059 See also (MY)
WD0101+866 See Also (PR)
WD0101-182 See also (QC)
WD0103-013 See also (RF)(RS)
WD0104-102 Shortest period (39.1 min) detached WD binary system known. Ref.(SU)
WD0104-464 BPM30551 is a ZZ CETI variable, Ref.(2W)(7I). See also (PB)
WD0106-328 See also (PS)(PP)
WD0106-358 Possible companion Finding chart for GD 683B see A4.2 in Ref.(LJ) See also (PP)(RK)
WD0107+131 WD/MS eclipsing binary system. Ref.(PH) See also (NC)(QH)(QN)
WD0108+000 ZZ Ceti star Ref.(KB)
WD0108+143 See also (PP)(OK)
WD0108+277 Cool Da with no metal features C. Melis 2008 private communication See also (PV)(PS)(OJ)
WD0108-001 See also (QJ)(NC)
WD0108-014 See also (QJ)
WD0108-106 See also (NC)
WD0110-139 See also (PP)
WD0110-162 See also (PP)
WD0111+002 See also (QP)
WD0111-102 See also (RF)(RS)
WD0112+132 See also (NC)
WD0113+006 See also (NC)
WD0114+002 See also (NC)
WD0115+159 G033-049 has strong UV absorption features, Ref.(BO)(NB) See also (PO)(OJ).
WD0116-231 Name(s) for MS companion(s). GD 695B See also (QP)
WD0120+154 See also (NC)
WD0120-024 See Also (PR)
WD0121-006 See also (QJ)
WD0121-429 Magnetic DA+DC double degenerate. Ref.(MD)(NY) See also (OJ)
WD0121-756 See also (JV)(KL)(SM)
WD0122+200 Pulsating PG1159 DO degenerate, Ref.(DN)(39); TYPE A, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
WD0124-257 See also (PP)
WD0126+101 Double degenerate system. Ref.(JP) See also (PP)(MM)(NB)(OL)(RQ)
WD0127+581 The DAO central star of the planetary nebula Sh2-188, Ref.(7U)
WD0127-311 HE0127-311 is a magnetic degenerate, Ref.(3W).
WD0128-012 See also (NC)
WD0128-387 MCT0128-3846 is an unresolved DA + DB or DBA binary. (DM)
WD0129-205 See also (PP)
WD0130+128 See also (QJ)(NC)
WD0130+141 See also (NC)
WD0130-196 MCT0130-1937 is a PG1159 star with no detected variability, type A, Ref.(66).
WD0130-273 See also (PP)
WD0131-163 See Section A5.16 in Ref.(LJ) See also (QP)(PP)(JV)(MQ)(MY)(NL)(RK)
WD0131-287 ZZ Ceti candidate (HC)
WD0132+127 Spectrum shows Mg I, Ref.(JJ)
WD0133-116 R548 is a ZZ CETI variable, Ref.(5C) See also (PP)(NL)
WD0133-299 ZZ Ceti candidate (HC)
WD0134+181 See also (JE)
WD0134+833 See also (QP)(NB)(NL)
WD0134-002 See also (QJ)(NC)
WD0135+002 See also (QJ)
WD0135-052 LP870-2 is a close detached DA binary system, Ref.(9K) Radial velocities -16.6/-41.2 km/sec Ref.(JP)N See also (NL)(OE)(OJ)
WD0136+251 Hot, low field magnetic ultra-massive DA star, Ref.(5V) See also (OQ)(9U)(JV)(NL)(RK)
WD0136+768 Double-degenerate system. Ref.(QX).
WD0136-201 Single-lined double-degenerate binary. Ref.(PP)
WD0137-004 See also (NC)
WD0137-349 Binary system consisting of a DA and a very low-mass detached companion. Ref.(RO).See also (QH)(SE)
WD0139+143 See also (NC)
WD0139+513 NGC650-1 is a PG1159 star with no detected variability and an associated planetary nebula, type E, Ref.(66).
WD0139-011 See also (QJ)(NC)
WD0140+130 See also (MV)
WD0141-675 See also (OJ)(MV)(MM)(OL)(RQ)
WD0143+216 See also (PP)(MY)
WD0145-174 See also (NN)
WD0145-221 ZZ Ceti star ref.(JT) Has a possible Brown Dwarf Companion ref.(KX) See also (QP)(PP)
WD0145-257 Name(s) for MS companion(s). GD1401B See also (QP)
WD0146+187 See also (QA)(PS)
WD0147+674 See also (RK)
WD0148+467 1400A absorption feature, Ref.(CL) Member of binary or multiple star system. Ref.(OJ) See also (PV)(PO)(NB)(NL)
WD0148+641 GR268 common proper motion binary with G244-37 (M2 DWARF), Ref.(1R).
WD0149-012 See also (NC)
WD0149-082 See also (NC)
WD0150+001 See also (NC)
WD0150+007 See also (PY)
WD0150-089 See also (PE)
WD0151+017 See also (PP)
WD0151-308 See also (QV)
WD0154-071 See also (QC)
WD0155+003 Spectrum shows Mg I, Ref.(JJ)
WD0155+069 See also (PS)
WD0156+155 See also (PS)
WD0158+235 A new hot DO with ultra highly excited ionization stages, Ref.(64).
WD0158-160 Composite DBA + dM binary, Ref.(DP).
WD0159-032 WD0159-032 is a magnetic degenerate, Ref.(02).
WD0201+004 See also (NC)
WD0201-006 See also (NC)
WD0201-052 See also (PP)
WD0202-055 See also (PF)
WD0203+007 Reclassified as carbon star; Ref.(QB)See also (NC)
WD0203+131 See also (NC)
WD0203-010 See also (NC)
WD0203-138 See also (PP)
WD0204-233 See also (PP)
WD0204-306 CPM Binary with LP885-923 (WD+dM) Ref.(MK)(PR)
WD0205+000 See also (NC)
WD0205+133 Name(s) for MS companion(s). PG 0205+133B See also (QR)(QP)
WD0205+250 See also (NL)
WD0205-297 Double-lined double-degenerate binary. Ref.(PP)
WD0208+002 See also (PD)(MV)
WD0208+396 G74-7 is the first known example of a definite DA, F degenerate, REF.(37),See also (QV)(QA)(MR)(NN)(RT)
WD0208-153 Name(s) for MS companion(s). MRT 0208-1520B
WD0208-510 CMPB with the dK1 Gliese 86; the WD Gl 86B Should not be confused with the exolanet GJ86b. Ref.(SB).See also (RZ)
WD0209+085 DAB star in the DO-DB gap, Ref.(63), Teff=36,000K, Ref.(3X),(63) See also (QP)(PP)
WD0209+210 See also (PD)(MV)
WD0210+000 See also (NC)
WD0210+086 White dwarf companion to the mild barium star XI 1 CETI; DA4 with 1400 and 1690 features, Ref.(37). Coords corrected, formerly WD0207+083
WD0210+138 See also (NC)
WD0210+168 See section A1.3 in Ref. (LJ).
WD0210-010 See also (NC)
WD0211+010 See also (QJ)(NC)
WD0211-086 ZZ Ceti star Ref.(KB) See also (NQ)
WD0212+140 See also (NC)
WD0213+396 See also (MY)
WD0213+427 See also (OJ)(NN)
WD0214+568 See also (MZ)(NL)
WD0214-007 See also (QJ)(NC)
WD0215+005 See also (QJ)(NC)
WD0215+006 See also (QJ)(NC)
WD0216+007 See also (NC)
WD0216+143 See also (QP)(PP)(JE)
WD0216+387 See also (PQ)
WD0216-005.1 See also (QJ)(NC)
WD0216-032 Luminosity of white dwarf probably dominated by wind accretion energy, Ref.(BX)(JV)(SM).
WD0217+003 See also (QJ)
WD0218+000 See also (NC)
WD0219+282 Has an Unresolved companion DA1.9 White Dwarf with (Vmag = 18.16 AbsMag = 10.32) Ref.(QC) Triple-star system: (DA+DB)+dM5 companion. Ref.(QO)(SG)
WD0220+222 See also (PP)(PQ)(SM)
WD0221+399 SEE also (PR)
WD0221+399 CPM Binary with BD+39 0539 (WD+dM) system. Ref.(MK)
WD0222+006 See also (QJ)(NC)
WD0222+422.1 CPM WD component with Mv > 15.0, Ref.(3A).
WD0222+422.2 CPM WD component with Mv > 15.0, Ref.(3A).
WD0222+648 Mv > 15.0, Ref.(51) formely WD0222+641.
WD0222-291 We obtain T=3000 K, this may be the coolest WD known. (JW).
WD0225-192 Double-lined double-degenerate binary. Ref.(PP)
WD0226-078 See also (QJ)
WD0227+001 See also (QJ)
WD0227+009 See also (NC)
WD0227+050 See also (PP)(NB)(NL)
WD0228-009 See also (NC)
WD0228-085 DB; binary nature questionable.Ref.(QB)See also (NC)
WD0229+270 See also (QC)
WD0230+343 See also (RY)
WD0230-144 See also (PV)(OJ)
WD0231-054 See also (MY)(NL)
WD0232+035 FEIGE 24 is an EUV source, PCEB, DAQZ+dwarf M2, Ref.(RV)(5Y) See also (QH)(PP)(NL)(RX)(SM).
WD0232+525 See also (NL)
WD0232-003 See also (QJ)(PJ)(NC)
WD0233-083.1 See also (MV)
WD0233-242 See also (OJ)
WD0234-012 See also (NC)
WD0235+064 CPMB system (DAZ+dM3.5 companion). Ref.(PS)See also (QA)
WD0235-003 See also (QJ)(NC)(QH)
WD0235-125 See also (RL)(RK)
WD0236+498 See also (NO)(RK)
WD0237+105 Single-lined double-degenerate binary. Ref.(PP)
WD0237+115 Name(s) for MS companion(s). PG 0237+115B
WD0239+109 G4-34 is a probable unresolved DA + DB binary, Ref.(23).
WD0240+004 See also (QJ)(NC)
WD0242+002 See also (QJ)(NC)
WD0242+009 See also (QJ)(NC)
WD0243-026 See also (QV)(QA)(OJ)(MR)(RT)
WD0244+004 PCEB. Ref.(QH) See also (QJ)(NC)
WD0245+541 See also (QA)(OJ)(MR)(RT)
WD0246+326 ZZ Ceti star ref.(GX)
WD0246-301 ZZ Ceti candidate (HC)
WD0247+053 A new DBA star from the HS survey, Ref.(4B)
WD0248-014 See also (NC)
WD0249-002 See also (NC)
WD0250-007 CPMB with BD-01 0407 Ref.(EP), Referenced as 0250-008 in Ref.(MK)(PR)
WD0251-008 See also (PQ)
WD0252-009 See also (NC)
WD0252-055 EUVE-discovered hot DA companion to the K0 IV star HD18131, Ref.(4D),(BP).
WD0252-350 See also (PP)
WD0253+508 New magnetic degenerate, Ref.(61).
WD0253-070 See also (NC)
WD0253-077 See also (QJ)(NC)
WD0255+006.1 See also (NC)
WD0255+009.2 See also (NJ)(NC)
WD0255-007 See also (PJ)(NC)
WD0255-110.1 See also (PP)
WD0255-705 See also (PP)(OJ)(MV)(NB)(NL)
WD0256-014 See also (QJ)
WD0257+080 See also (MV)
WD0257-005 Name(s) for MS companion(s). KUV 02579-0036B See also (QP)
WD0257-075 See also (RF)(RS)
WD0259+004 See also (NC)
WD0300+007 WD/MS eclipsing binary system. Ref.(PH) See also (PH)(NC)
WD0300-008 See also (QJ)
WD0300-013 A DB degenerate with calcium, Ref.(AC). See also (QD)(QA)(PZ)(OR)(RF)(RS)
WD0300-066 See also (NC)
WD0301+004 See also (QJ)(NC)
WD0301-006 See also (PD)(MV)
WD0302+027 See also (QP)(PP)(NL)(RK)
WD0302+621 See also (MU)
WD0303-007 Name(s) for MS companion(s). KUV 03036-0043B See also (QP)
WD0303-080 See also (QJ)(NC)
WD0304+004 See also (NC)
WD0304+154 See also (JV)
WD0306-006 See also (QJ)(NC)
WD0306-012 See also (NC)
WD0307+077 See also (QV)(MR)
WD0307-428 WD0307-428 is a magnetic degenerate, Ref.(02).
WD0308+096 The dM companion is likely a binary M2 dwarf, see A5.19 in Ref.(LJ) See also (QX)(QX)(QH)
WD0308+188 See also (QP)
WD0309-005 See also (NC)
WD0309-275 Name(s) for MS companion(s). WD 0309-75B
WD0310-073 See also (OK)
WD0310-688 1400A absorption feature, Ref.(CH) See also (PP)(NB)(NL)(OE)(OK)
WD0311-013 See also (QJ)(NC)
WD0313-066 See also (OY)
WD0315-011 CPMB WITH BD-01 0469 See also (OS)
WD0315-013 Double-lined double-degenerate binary. Ref.(PP)
WD0316+003 ZZ Ceti star Ref.(KB)
WD0316-003 See also (NJ)
WD0316-849 RE0317-853 is a magnetic degenerate, Ref.(3Z).
WD0317-011 See also (NC)
WD0318-068 See also (QJ)(NC)
WD0319-004 See also (QJ)(NC)
WD0320-000 See also (OK)
WD0320-192 Single-lined double-degenerate binary. Ref.(PP)
WD0320-539 See also (PP)(JV)(NL)(RK)
WD0321-002 See also (QJ)(NC)
WD0321-009 Reclassified as QSO; Ref.(QB)
WD0322+452 The DAO central star of HDW3, Ref.(7U).
WD0322-013 See also (NC)
WD0322-019 Double degenerate system. Ref.(JP)(NN) See also (QA)(OJ)
WD0323+009 See also (NC)
WD0324+738 RA=033013.89 Dec=+740157.1(2005.09), resolved triple (WD+dM5+dM6) system. Ref.(MQ) See also (QP)
WD0324-012 See also (NC)
WD0324-012.1 See also (NC)
WD0324-197 Double-lined double-degenerate binary. Ref.(PP)
WD0325-005 See also (QJ)(NC)
WD0325-405 Single-lined double-degenerate binary. Ref.(PP)
WD0325-857 LB 9802 is the visual companion to the high-field ultramassive WD EUVEJ0317-85.5, separation ~ 200AU. Ref.(MV)See also (RL)
WD0326+001 See also (NC)
WD0326-273 Double degenerate system; radial velocities 105.9/157.1 km/sec Ref.(JP) See also (PV)(OJ)(PR)
WD0328+008 See also (PP)(PM)(OK)
WD0328-010 See also (NC)
WD0329+005 KUV03292+0035 is a magnetic degenerate, Ref.(3V). This star is listed at Dec -00 35.1 in Ref.(CP). See also (PD)
WD0330-000 See also (PD)
WD0330-009 See also (OK)
WD0330-009.1 ZZ Ceti star Ref.(KB)
WD0330-013 See also (NC)
WD0331-356 Name(s) for MS companion(s). HE 0331-3541B See also (SM)
WD0333+004 See also (QJ)(NC)
WD0333-350 See also (JV)
WD0334-002 See also (NJ)
WD0334-009 See also (QJ)(NC)
WD0335-002 See also (QJ)(NC)
WD0335-420 See also (RK)
WD0337+096 Hot/cold Table 1 temperatures ambigious. Ref.(PP)
WD0338+007 See also (MS)
WD0339+002 Has an Unresolved companion DB3.7 White Dwarf with (Vmag = 17.82 AbsMag = 11.57) Ref.(QC)
WD0339-035 Temperatures ambigious. Ref.(PP)
WD0339-451 See also (JV)(SM)
WD0340+009 See also (QJ)(NC)
WD0340-068 See also (PD)(MV)
WD0340-075 See also (MS)(NR)
WD0341+021 Variability in radial velocity indicates a long period binary. (EE) Single-lined double-degenerate binary. Ref.(PP)
WD0341+182 See also (PV)(OJ)(NN)
WD0341-076 See also (NC)
WD0341-459 BPM31594 is a ZZ CETI variable, Ref.(7H). See also (PB)
WD0342+004 See also (PD)(MV)
WD0342+176 Double-degenerate merger system. Ref.(QT).
WD0342+374 Hot DA planetary nucleus, Ref.(7U).
WD0343+247 An ultra cool White Dwarf referred to in the references as WD0346+246
WD0343-007 See also (PP)
WD0344+014 See also (OJ)
WD0344+073 Long period ZZ Ceti (OC) single-lined double-degenerate binary. Ref.(PP)
WD0344-121 See also (PP)
WD0345+006 See also (RY)
WD0345+498 IW1 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(DI); type A Ref.(66).
WD0346-011 See also (PP)(OQ)(MY)(MZ)(NL)(RK)
WD0346-063 See also (QJ)(NC)
WD0347+171 V471 TAU,HYADES DA and K0V Eclipsing and Spectroscopic binary, REF(7V). DA star has TEFF=32,500K, LOG G=8, Ref.(2N)(JV). See also (PH)(SM)
WD0347-137 Name(s) for MS companion(s). GD 051B See also (QP)
WD0348+339 See also (NL)
WD0348-066 See also (NC)
WD0349+247 Pleiad white dwarf with mass 0.98 MSUN; VGRAV= +84+/- 9 KM/S, Ref.(CR) See also (OS)(OQ)(MZ)
WD0350-002 See also (NC)
WD0352+049 See also (PP)
WD0352+096 The finding charts point to different stars. See also (PP)(OS)(OQ)(MZ)(NL)
WD0354+463 See section A5.25 in Ref. (LJ), (MQ) See also (QP)
WD0355+255 SEE also (PR)
WD0357+081 See also (PF)(OJ)
WD0357-233 Name(s) for MS companion(s). Ton S 392B See also (QP)
WD0358-051 DA with odd H-Alpha emission; Ref.(QB)See also (NC)
WD0400-346 CMPB with the G1/2 V double star HIP 18824. Ref.(SH)
WD0401+149 Temperatures ambigious. Ref.(PP)
WD0401+250 See also (NL)
WD0406+169 See also (OS)(OQ)(NL)
WD0408-041 Contains circumstellar dust (NG) See also (QV)(QD)(QA)(PS)(PP)(OR)(MR)
WD0410+117 See also (QP)(PP)(NL)
WD0410-116 Double-lined double-degenerate binary. Ref.(PP)
WD0413-077 The mass of 40ERI B is 0.43 MSUN, Ref.(8K). 1400A absorption feature, Ref.(2A) CPMB with K1 V star HD 26965. Ref.(OF) See also (OS)(NL)(OK)(OJ)(RX)
WD0415+271 HL TAU76 is a ZZ CETI variable, Ref.(4X). See also (PB)(OQ)
WD0415-594 Sirius-like system. Ref.(RZ) CMPB with HD 27442A; the WD HD 27442B should not be confused with the exoplanet HD 27442b. Ref.(SA).
WD0416+334 Finding chart for GD 60B Ref.(LJ)
WD0416+402 See also (NO)
WD0416-550 See also (PP)(JV)
WD0417+361 G038-029 is a ZZ CETI variable, Ref.(7L). See also (PB)
WD0418+137 Companion to HR 1358, a F6V spectroscopic binary. Ref.(EX)(SM)
WD0419-487 Eclipsing system, WD + Red dwarf. See also (PH)(OJ)(MV)(QH)(SM)
WD0420-007 See also (NC)
WD0421+162 See also (PP)(OS)(OQ)
WD0421+338 A quadruple system. (EX)
WD0421+740 See also (QM)(RK)
WD0422+543 See also (QX)
WD0425+168 See also (QP)(PP)(OS)(OQ)(JV)(NL)
WD0426+588 The mass of this star is 0.48 or 0.68 MSUN, Ref.(AW)(JV)(NN) See also(OJ).
WD0429+176 White dwarf-red dwarf Hyades spectroscopic binary, REF(5B). DA white dwarf with T=20,000K, LOG G=8, Ref.(AR)(JV). See also (QH)(PP)(SM)
WD0430+136 Name(s) for MS companion(s). KUV 04304+1339B/C. Triple-star system: Unresolved DA+dM4e binary and a dM5.5e companion. Ref.(QO)
WD0431+126 See also (PP)(OS)(OQ)
WD0433+270 EG40 common proper motion binary with G39-27 / BD+26 0730 (K5 DWARF), Ref.(7Z) See also (PV)(OJ)(PR).
WD0435+410 See also (OB)
WD0435-088 See also (OJ)(NN)
WD0437+138 See also (OS)(OQ)
WD0438+108 See also (QC)(OS)(OQ)(RY)
WD0439+466 DAO nucleus of the planetary nebula S216, Ref.(7U).
WD0440-038 See also (OQ)(JV)(RK)
WD0443-275.1 Very close common proper motion pair, Ref.(7Z)(PR).
WD0444+049 New PG1159 star, type A, Ref.(66).
WD0446-789 See also (JV)(NB)
WD0449-259 See also (OR)
WD0453+418 See also (NL)
WD0453-295 A rare DAB hybrid composition degenerate, Ref.(DP), MCT0453-295 is an unresolved DA + DB binary, Ref.(DM).
WD0455+553 GR318 is a ZZ CETI variable, Ref.(7J). See also (PB)
WD0455-282 A new hot DA in a region of extremely low HI density, Ref.(15) See also (NB)(NL)(RK)
WD0455-532 single-lined double-degenerate binary. Ref.(PP)
WD0457-004 See also (OJ)
WD0457-103 K0IV + DA binary, Ref.(14).
WD0458-665 X-ray selected hot DA + dM(RX J0458.9-6628B) binary, Ref.(3P)(SM).
WD0500-156 The DAO central star of ABELL 7, Ref.(7U).
WD0501+527 See also (QP)(PM)(NL)(OK)(RX)
WD0501-289 Evidence of episodic mass ejection, rich metallic EUV spectrum, Ref.(DK,DT).
WD0503-174 LHS1734 is a magnetic degenerate, Ref.(27)(MV) See also (PF)(OJ).
WD0504-241 DO white dwarf with ultra-high excitation absorption, Ref.(31).
WD0507+045.1 One component of a visual pair of DA stars, Ref.(63), ZZ Ceti star ref.(IY) See also (PB)
WD0507+045.2 One component of a visual pair of DA stars, Ref.(63). See also (QP)(PP)
WD0509-007 See also (PP)(MV)(NL)(RK)
WD0510-418 See also (PP)(RK)
WD0512+326 System of 4 stars; primary and tertiary components are spectroscopic binaries. Ref.(SI) See also (RK)(SM)
WD0513+260 V1063 TAU is a non-radial pulsator, Ref.(44). See also (PB)
WD0517+307 GD 66 is a ZZ CETI variable, Ref.(57). See also (PB)
WD0517+357 PCEB. Ref.(QH).
WD0518+333 Name(s) for MS companion(s). G086-B1A/C. Triple-star system: DA and a binary (dM3+dM3) proper motion companion. Ref.(QO)(PQ)
WD0518-105 See also (OQ)(JV)(RK)
WD0531-022 See also (JV)
WD0532+414 Double degenerate system; radial velocities -38/150 km/sec Ref.(JP) See also (OJ)
WD0532-560 ZZ Ceti star ref.(JT)
WD0533+555 DA central star of the planetary nebula HDW4, Ref.(7U).
WD0543+579 See also (MR)
WD0548+000 See also (PP)(JV)(NL)(RK)
WD0548+326 See also (OS)
WD0548+326.1 See also (OS)
WD0548-001 G99-37 is magnetic and polarized, Zeeman H alpha, Ref.(5H)(03) See also (PV)(MV)(OJ).
WD0548-241 See also (RK)
WD0549+158 See also (PP)(PM)(MV)(MZ)(NB)(NL)(RK)
WD0549+324 See also (OS)
WD0549+324.1 See also (OS)
WD0549+325.1 See also (OS)
WD0549+325.2 See also (OS)
WD0549+325.3 See also (OS)
WD0549+325.4 See also (OS)
WD0549+325.6 See also (OS)
WD0549+325.7 See also (OS)
WD0549+326.1 See also (OS)
WD0549+326.2 See also (OS)
WD0551+123 CMPB with the F8 star HIP 27878. Ref.(SH)
WD0552-041 See also (PC)(OJ)(MM)(NB)(NN)(OL)(RQ)(1V)
WD0553+053 G99-47 is a magnetic white dwarf, Ref.(03) See also (OL)(MV)(MM)(NB)(NN)(OJ)(RQ).
WD0556+106 Rare DA nucleus of planetary nebula with Teff > 1E+5K, Ref.(5J).
WD0558-756 Helium-rich DO nucleus of K1-27; TEFF>1E+5;similar to KPD0005, Ref.(8O)(JV).
WD0603-483 See also (NO)(RK)
WD0605+241 NGC2168:LA 2 = NGC2168:LAWDS 2
WD0605+242 See also (OS)
WD0605+245 NGC2168:LA22 = NGC2168:LAWDS22 See also (OS)
WD0606+240 NGC2168:LA15 = NGC2168:LAWDS15 See also (OS)
WD0606+241 NGC2168:LA11 = NGC2168:LAWDS11
WD0606+243 NGC2168:LA27 = NGC2168:LAWDS27
WD0606+244.1 NGC2168:LA 5 = NGC2168:LAWDS 5 See also (OS)
WD0606+244.2 NGC2168:LA 6 = NGC2168:LAWDS 6 See also (OS)
WD0612+177 G104-27 detection of trace helium in a DA star, Ref.(3K) See also (PP)(NL)
WD0615+556 Central star of the planetary nebula PW1, Ref.(7U).
WD0615-591 CPMB WITH CD-59 1275 See also (PR)
WD0616-649 RE0616-649 is a new magnetic degenerate, Ref.(4A).
WD0621-376 See also (QP)(PP)(MV)
WD0622-329 Unresolved DA/DB double degenerate Ref.(MD)
WD0625+415 Finding chart for GD 74B see A5.13 in (LJ)
WD0625-253 Central star of Abell 15, REF.(2B).
WD0630-050 See also (PP)(RK)
WD0631+107 See also (RK)
WD0637+477 GD77 is a magnetic degenerate, Ref.(9X) See also (MV)
WD0640+015 Cool DO star (TEFF = 55000K) with one of the strongest HeII 4686 absorption lines of any known star, Ref.(7C)(5Q).
WD0642-166 SIRIUS B mass=1.02 MSUN, Ref.(BK) See also (OS)(OJ).
WD0642-285 CPMB WITH CD-28 3358 See also (PR) (P.Bergeron Finding Chart)
WD0644+025 See also (OJ)
WD0644+375 See also (OJ)(NB)(NL)
WD0646-253 See also (MV)(RK)
WD0651-020 See also (JV)(NL)(RK)
WD0652-563 See also (OQ)(RL)
WD0657+320 See also (OJ)
WD0659-063 Listed in ref (NN) as WD0659-064 See also (OJ)
WD0704+618 Coolest PG1159 star, no detected variability, Ref.(2T); type A, Ref.(66).
WD0708-670 See also (PV)
WD0710+216 See also (PP)
WD0710+741 See also (QH)
WD0713+399 A new DO star with ultra-highly excited ionization features, Ref.(31)
WD0713-468 LONGMORE 3 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(7R)(KL).
WD0714+458 Possible companion 0714+458 Finding chart for GD 84B see A4.1 in Ref.(LJ)
WD0715-703 See also (JV)(MV)(NB)(RK)
WD0718-316 DAO+dM2 pre-cataclysmic binary. Ref.(IT) See also (QM)(QH)(MV)(RK)
WD0721-276 See also (MV)(RK)
WD0726+133 ABELL 21 is a PG1159-like star with no detected variability and an associated planetary nebula Type E, Ref.(DG)(KL).
WD0726+392 See also (PR)
WD0727+376 See also (NC)
WD0727+482 G107-70 consists of a close pair of DC stars, it is also a widely seperated CPM pair with a red subdwarf(G107-069) Ref.(AX)(NN) See also (OJ).
WD0727+600 A new intermediate temperature DO star with ultra-highly excited species, Ref.(2T).
WD0728+642 P. Bergeron reports his spectra does not show Zeeman splitting, Private Communication 3/11/2010 See also (OJ)
WD0729+397 See also (NC)
WD0730+487 See also (OQ)
WD0732+330 See also (NC)
WD0732-427 (P.Bergeron Finding Chart)
WD0733+389 See also (NC)
WD0733+468 MS+MS superposition; Ref.(QB)
WD0734-143 See also (JV)
WD0736+053 PROCYON B has mass =0.63 MSUN, Ref.(AV)(JV) See also (OJ)(SM).
WD0736+278 See also (NC)
WD0736+391 See also (NC)
WD0737-384 Member of the open cluster NGC 2451, Ref.(4O). (P.Bergeron Finding Chart)
WD0738+222 See also (NC)
WD0738+283 See also (RS)
WD0738+382 See also (NC)
WD0738+418.1 See also (NC)
WD0738-172 First detection of calcium two 1840A absorption in a white dwarf, Ref.(4L)(NN) LHS 234 M6.0V CPM companion(PC) See also (QA)(PO)(OJ).
WD0738-382 Member of the open cluster NGC 2451, Ref.(4O).
WD0739+238 See also (NC)
WD0739+412 See also (NC)
WD0740+325 See also (NC)
WD0740+348 See also (NC)
WD0741+248 See also (PR)
WD0741+356 See also (NC)
WD0742+231 See also (OK)
WD0742+238 See also (NC)
WD0742+653 A new intermediate temperature DO star, Ref.(2T).
WD0743+442 See also (MY)
WD0743+474 See also (NC)
WD0743-336 VB3 common proper motion with HD63077 (G0 DWARF), shown to be low luminosity DC9 degenerate, not an M dwarf, Ref.(4T). (P.Bergeron Finding Chart) See also (OJ)
WD0744+382 See also (NC)
WD0744+384 See also (NC)
WD0744+431 See also (QJ)(NC)
WD0745+210 See also (NC)
WD0745+247 See also (QJ)(NC)
WD0745+258 See also (NC)
WD0745+304 See also (PD)(MV)
WD0745+436 See also (NC)
WD0746+384 See also (NC)
WD0746+396 See also (NC)
WD0746-375 Member of the open cluster NGC 2451, Ref.(4O).
WD0747+073.1 LHS 239 and LHS 240 are double DC white dwarfs, Ref.(5M)(NN) See also (OJ).
WD0747+073.2 LHS 239 and LHS 240 are double DC white dwarfs, Ref.(5M)(NN) See also (OJ).
WD0747+247 CPMB with WD 0747+247.1 Ref.(QL).
WD0747+247.1 CPMB with WD 0747+247 Ref.(QL).
WD0748+230 See also (NC)
WD0748+436 See also (NC)
WD0749+426 See also (PV)(OJ)
WD0750+267 See also (NC)
WD0750+317 See also (NC)
WD0750+379 See also (NC)
WD0751+299 See also (NC)
WD0751-252 See also (OJ)
WD0751-595 Foreground star not a cluster member, Ref.(8S).
WD0752+278 See also (NC)
WD0752+398 DA with very noisy spectrum; Ref.(QB)See also (NC)
WD0752+402 See also (MS)(NR)
WD0752+424 See also (NC)
WD0752+492 Double-degenerate merger system. Ref.(QT).
WD0752-146 Slight variability in radial velocity indicates a possible binary. Emission line has a VR0= -146.8km/s. (EE) See also (QP)
WD0752-676 See also (OL)(OJ)(RQ)
WD0753+313 See also (NC)
WD0753+478 See also (NC)
WD0753+535 VV47 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(5O)(1M); type E, Ref.(66).
WD0754+326 See also (QJ)(NC)
WD0754+402 See also (OK)
WD0755+358 See also (PD)(MV)
WD0756+324 See also (NC)
WD0756+350 See also (NC)
WD0756+437 A new magnetic degenerate with a 220 MG field, Ref.(8N).
WD0756+493 See also (NC)
WD0756-607 Foreground star not a cluster member, Ref.(8S).
WD0757+075 See also (QJ)
WD0757+118 See also (QJ)
WD0757+501 See also (NC)
WD0757-603 Member of the open cluster NGC 2516, Ref.(8S).
WD0757-606.1 Member of the open cluster NGC 2516, Ref.(8S).
WD0757-606.2 Member of the open cluster NGC 2516, Ref.(8S).
WD0758+224 See also (NC)
WD0758-476 See also (JV)
WD0800+233 See also (NC)
WD0800+417 See also (NC)
WD0801+186 See also (PD)(MV)
WD0801-608 Foreground star not a cluster member, Ref.(8S).
WD0802+220 See also (PD)(MV)
WD0802+386 See also (OR)
WD0803+340 See also (NC)
WD0803+407 See also (NC)
WD0804+075 See also (QJ)(NC)
WD0804+397 See also (MV)
WD0805+185 See also (QJ)
WD0805+654 See also (JV)
WD0806+312 See also (RS)
WD0806+376.1 See also (PD)(MV)
WD0806-661 L0097-003 shows strong UV CI absorption, Ref.(DD) See also (OJ).
WD0807+190 Probably a moderate velocity red dwarf. private comm. J.Farihi 9/2008
WD0807+416 See also (NC)
WD0807+463 Reclassified as M star; Ref.(QB)See also (NC)
WD0807+484 See also (PR)
WD0808+058 See also (QJ)(NC)
WD0808+272 See also (MT)
WD0809+034 See also (NC)
WD0809+235 See also (NC)
WD0810+234 See also (PQ)
WD0810+329 See also (NC)
WD0810+455 See also (NC)
WD0810+489 See also (OJ)
WD0810-728 See also (PP)(RK)
WD0811+111 WD+MS Eclipsing Binary System. Ref.(QN).
WD0811+411 See also (NC)
WD0811+414 See also (NC)
WD0812+208 See also (QJ)
WD0812+433 See also (NC)
WD0812+436 WD/MS binary nature questionable. Ref.(QB)
WD0812+447 ZZ Ceti star Ref.(KB)
WD0812+478 Name(s) for MS companion(s). PG 0812+478B
WD0813+265 See also (NC)
WD0813+358 See also (NC)
WD0814+001 See also (QJ)
WD0814+043 See also (PD)(MV)
WD0814+058 See also (QJ)(NC)
WD0814+271 See also (NC)
WD0815+176 See also (QJ)
WD0815+357 Double-degenerate merger system. Ref.(QT)(QS).
WD0816+356 See also (NC)
WD0816+376 GD90 magnetic, not polarized, Zeeman H lines, Ref.(05)(03).
WD0816+433 Post-common envelope binary. Ref.(QB)See also (QJ)(NC)
WD0816-310.1 See also (OJ)
WD0817+062 See also (QJ)(NC)
WD0817+255 See also (NC)
WD0818+461 See also (NC)
WD0819+280 Double-degenerate merger system. Ref.(QT)(SL).
WD0819+355 See also (NC)
WD0819+461 See also (NC)
WD0820+250.1 See also (PM)
WD0821+175 See also (QJ)
WD0821+275 See also (NC)
WD0821-252 See also (RK)(OQ)(MV)
WD0821-669 See also (PV)(OJ)
WD0822+036 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD0822+342 See also (NC)
WD0822+414 ZZ Ceti star Ref.(KB)
WD0823+039 See also (NC)
WD0823+062 DA; binary nature questionable. Ref.(QB)See also (NC)
WD0823+316 Central star of PN. Ref.(QM) See also (QP)
WD0823+336 See also (NC)
WD0824+066 DA; binary nature questionable. Ref.(QB)See also (NC)
WD0824+082 Reclassified as M star; Ref.(QB)See also (NC)
WD0824+288 Double lined spectroscopic binary, DA + dwarf carbon star, Ref.(2R). dC companion VR0 = -36.8(EE) Triple system: DA+dC+M3V (IH)(JV), see A5.4 Ref.(LJ) See also (QO)(QP)
WD0824+474 See also (NC)
WD0825+072 DA; binary nature questionable. Ref.(QB)See also (NC)
WD0825+297 See also (PD)(MV)
WD0826+271 See also (NC)
WD0826+282 DA binary nature questionable. Ref.(QB)See also (NC)
WD0827+080 Reclassified as M star; Ref.(QB)
WD0827+291 See also (NC)
WD0827+321 See also (NC)
WD0827+368 DA; binary nature questionable Ref.(QB)See also (NC)
WD0827+410 See also (RY)
WD0827+472 See also (NC)
WD0828+081 Reclassified as MS + bright star; Ref.(QB)
WD0828+412 See also (NC)
WD0830+536 See also (NC)
WD0830-535 See also (PP)(NO)(RK)
WD0831+056 See also (NC)
WD0831+072 See also (QJ)(NC)
WD0831+140 See also (QJ)
WD0832+436 See also (NC)
WD0833+049 Cataclysmic variable? Ref.(QB)See also (QJ)(NC)
WD0833+198 See also (OS)
WD0834+087 Reclassified as M star + star nearby; Ref.(QB)
WD0834+270 See also (NC)
WD0834+500 See also (JE)
WD0834+532 See also (NC)
WD0835+194 WD+MS Eclipsing Binary System. Ref.(QN).
WD0836+197 Praesepe member. See also (OS)
WD0836+199 Praesepe member. See also (OS)
WD0836+201 Praesepe member. See also (OS)
WD0836+237 See also (NL)
WD0836+404 ZZ Ceti star ref.(KA)
WD0837+189 See also (OS)
WD0837+199 Praesepe member. See also (OS)(MV)
WD0837+218 See also (OS)
WD0837+271 See also (NC)
WD0837+273 See also (MV)
WD0837+280 See also (NC)
WD0837+283 See also (NC)
WD0837+330 See also (MS)
WD0837+458 See also (NC)
WD0838+035 See also (JV)
WD0838+375 CBS78 is the second known DB star showing accreted calicium, Ref.(AN).See also (RS)
WD0839+025 See also (PD)(MV)
WD0839+086 See also (NC)
WD0839+179 MS+MS superposition; Ref.(QB)
WD0839+345 See also (OK)
WD0839+372 ZZ Ceti star Ref.(KB)
WD0839-327 See also (PV)(PP)(PC)(OJ)(MV)(MM)(NB)(NL)(OL)(RQ)
WD0839-528 Not a confirmed cluster member, Ref.(4O)(JV).
WD0840+047 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD0840+126 See also (QJ)
WD0840+190 See also (OS)
WD0840+200 Possible PRAESEPE member, Ref.(BV)(JV). See also (OS)
WD0840+209 See also (OS)
WD0840-136 See also (OJ)
WD0841+055 See also (NC)
WD0841+098 See also (NC)
WD0841+218 DA; binary nature questionable. Ref.(QB)
WD0842+375 See also (NC)
WD0842+490 See also (JV)
WD0843+058 DA; binary nature questionable. Ref.(QB)
WD0843+186 See also (OS)
WD0843+358 See also (OJ)
WD0843+488 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)
WD0844+287 See also (NC)
WD0844+453 ZZ Ceti star Ref.(KB) See also (NQ)
WD0845+011 See also (QJ)(NC)
WD0845+440 See also (NC)
WD0845-188 CPMB WITH CD-18 2482 See also (PR)
WD0846+006 See also (RF)(RS)
WD0846+049 Double-degenerate merger system. Ref.(QT).
WD0846+052 See also (QJ)(NC)
WD0846+081 DA; binary nature questionable.Ref.(QB)
WD0846+249 See also (JE)
WD0846+346 See also (QA)(MR)(OH)(RY)
WD0847+456 See also (NC)
WD0848+007 See also (QJ)(NC)
WD0848+037 See also (QJ)(NC)
WD0848+062 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD0849+049 Possible double-degenerate system. Ref.(SL)
WD0849+068 See also (NC)
WD0849+276 See also (QJ)
WD0849+319 See also (QX)
WD0849+549 See also (NC)
WD0850+472 See also (NC)
WD0850-617 (P.Bergeron Finding Chart)
WD0853+049 See also (QJ)(NC)
WD0853+057 See also (NC)
WD0853+069 See also (NC)
WD0853+163 Misidentified as LB 8827 in much of the literature (IW)
WD0854+158 See also (QJ)
WD0855+039 WD+MS Eclipsing Binary System. Ref.(QN).
WD0855+328 See also (NC)
WD0855+373 See also (NC)
WD0855+407 See also (NC)
WD0855+416 See also (PD)(MV)
WD0855+583 See also (NC)
WD0855+604.1 See also (PR)
WD0855+604.2 Possible CV? Ref.(AT). See also (PR)
WD0856+047 See also (QJ)(NC)
WD0856+331 EG182 common proper motion binary with HD77408 (F8 dwarf); G47-18 is a strong carbon band, DQ star polarized, Ref.(75). Section A2.1 in Ref(LJ) reports different motions for the pair therefore not CPMB. See also (OJ)
WD0856+577 See also (RS)
WD0857+001 See also (OY)
WD0857+086 See also (QJ)
WD0858+363 GD99 is a ZZ CETI variable, Ref.(7M) See also (PB)(NL)
WD0858+441 DA; binary nature questionable.Ref.(QB)See also (NC)
WD0859+337 See also (OK)
WD0859+391 Reclassified as carbon star; Ref.(QB)
WD0859-039 See also (MV)
WD0900+426 See also (NC)
WD0900+565 See also (NC)
WD0901+016 See also (OY)
WD0901+140 Visual double degenerate Finding chart for PG 0901+140B see A5.8 in Ref.(LJ)
WD0901+530 See also (OY)
WD0902+060 See also (QJ)
WD0902+097 See also (QJ)(NC)
WD0903+083 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) See also (MV)
WD0903+166 See also (JV)
WD0903-002 ZZ Ceti star Ref.(KB)
WD0904+358 See also (PD)(MV)
WD0904+511 See also (JV)
WD0905+062 WD/MS eclipsing binary system. Ref.(PH) See also (QJ)(NC)(QH)(QN)
WD0905+372 See also (NC)
WD0905+538 See also (QJ)(NC)
WD0905-724 See also (SM)
WD0906+006 See also (RF)(RS)
WD0906+076 See also (NC)
WD0906+296 See also (PR)
WD0908+033 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD0908+171 See also (PP)
WD0908+226 DA star, spectroscopic composite with dM(LP369-15B), Ref.(7Z). See also (QJ)
WD0908+422 See also (PD)(MV)
WD0910+014 See also (QJ)(NC)
WD0910+584 See also (MS)
WD0910+593 See also (NC)
WD0911+059 See also (PD)(MV)
WD0911+651 See also (PR)
WD0912+105 See also (NC)
WD0912+318 See also (NC)
WD0912+453 See also (NC)
WD0912+536 Polarization observed, Ref.(06) See also (PV)(PO)(OL)(MV)(NB)(NN)(OJ)(RQ)
WD0913+055 Propose that spectrum originates from two unrelated stars on same line of sight. Ref.(MS)
WD0913+408 See also (NC)
WD0913+442 EG64 common proper motion binary with G115-64 (G5 dwarf), Ref.(75). Section A2.1 in Ref(LJ) reports different motions for the pair therfore not CPMB See also (NZ)(PQ)
WD0913+444 See also (NC)
WD0913-003 See also (QJ)(NC)
WD0914+096 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD0914+610 See also (NC)
WD0914-195 See also (OQ)(JV)(RK)
WD0915+180 See also (QJ)
WD0915+201 Name(s) for MS companion(s). LB 3016B
WD0915+414 See also (NC)
WD0915+551 See also (NC)
WD0916+064 See also (OK)
WD0916+090 See also (NC)
WD0917+430 See also (NC)
WD0917-000 See also (NC)
WD0918+047 See also (NC)
WD0918+111 See also (NC)
WD0918+398 See also (NC)
WD0918+593 DA; binary nature questionable.Ref.(QB)See also (NC)
WD0919+003 See also (OY)
WD0919+104 See also (NC)
WD0920+015 ZZ Ceti star Ref.(KB)
WD0920+306 Double-degenerate merger system. Ref.(QT).
WD0921+012 See also (NC)
WD0921+016 See also (QJ)(NC)
WD0921+020 See also (NC)
WD0921+354 G117-B15A is a ZZ CETI variable, Ref.(7M) See also (PB)(8W)(JE)(NL)(PQ)
WD0922+006 See also (QJ)(NC)(QH)
WD0922+014 See also (PD)(MV)
WD0922+065 See also (NC)
WD0922+162 Double degenerate ref.(JE) See also (PP)
WD0922-000 See also (QJ)(NC)
WD0923+219 See also (QJ)
WD0924+337 See also (NC)
WD0925+386 See also (NC)
WD0925+498 DA; binary nature questionable.Ref.(QB)
WD0926+084 Hot/cold Table 1 temperatures ambigious. Ref.(PP)
WD0928+379 See also (NC)
WD0928+399 See also (NC)
WD0928+399.1 See also (NC)
WD0928-713 Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart
WD0929+350 See also (NC)
WD0929+380 DA?; binary nature questionable. Ref.(QB) See also (QM)
WD0930+096 See also (NC)
WD0930+294 See also (MY)
WD0930+815 A DA white dwarf companion to the hybrid K3II giant HD81817A See also (SM)
WD0931+034 See also (QJ)(NC)
WD0931+054 See also (QJ)(NC)
WD0931+058 See also (NC)
WD0931+105 See also (PD)(MV)
WD0931+444 See also (NC)
WD0931+507 See also (PD)(MV)
WD0932+230 WD+MS Eclipsing Binary System. Ref.(QN).
WD0933+025 Name(s) for MS companion(s). PG 0933+025B
WD0933+345 See also (NC)
WD0933+423 See also (NC)
WD0933+526 Spectrum shows Mg I, Ref.(JJ)
WD0933+729 Possible companion Finding chart for PG 0933+729B see A4.3 in Ref.(LJ)
WD0934+020 See also (RF)(RS)
WD0934+067 See also (NC)
WD0934-587 (P.Bergeron Finding Chart)
WD0935+577 See also (NC)
WD0935-371.1 Strong UV CI lines, Ref.(CK) See also (PR).
WD0935-371.2 Very close white dwarf pair; UBV photometry, Ref.(61) See also (PR).
WD0936+054 See also (QJ)(NC)
WD0936+331 WD+MS Eclipsing Binary System. Ref.(QN).
WD0936+378 See also (NC)
WD0936+382 See also (NC)
WD0936+560 See also (RF)(RS)
WD0936+563 ZZ Ceti star Ref.(KB)
WD0936+595 See also (NC)
WD0937+049 DA; binary nature questionable.Ref.(QB)See also (NC)
WD0937+505 See also (JV)(MZ)(NO)(OK)(RK)
WD0937+513 See also (NC)
WD0937+527 See also (NC)
WD0938+002 See also (NC)
WD0938+065.1 See also (QJ)
WD0938+550.1 See also (PM)
WD0938+577 ZZ Ceti star Ref.(KB)
WD0939+071 Spectra doesn't look like a single WD, P.Bergeron and J.Holberg, private comm 3/2008. See also (PS)(OJ)
WD0939+262 See also (QP)(NL)
WD0940+114 Hot/cold Table 1 temperatures ambigious. Ref.(PP)
WD0940+608 Possible sdOB/WD binary system. Ref.(QX).
WD0940+619 See also (QJ)(NC)
WD0941+432 See also (OK)
WD0941+458 See also (PD)(MV)
WD0942+236.1 See also (PR)
WD0942+236.2 See also (PR)
WD0943+441 See also (QP)(NL)
WD0944+115 See also (NC)
WD0944+424 See also (RY)
WD0944+452 has a common proper motion WD companion 20" away Ref.(KR)(OM)
WD0945+021 See also (OY)
WD0945+127 See also (NC)
WD0945+245 LB11146 is a magnetic DX degenerate in a double degenerate binary with a non-magnetic DA companion, Ref.(5I) See also (QP)(JE)(MV).
WD0945+372 See also (NC)
WD0945+578 See also (QJ)(NC)
WD0946+002 ZZ Ceti star Ref.(KB)
WD0946+020 See also (NC)
WD0946+036 See also (QJ)(NC)
WD0946+488 See also (NC)
WD0946+534 See also (OJ)
WD0947+016 See also (NC)
WD0947+452.1 CPMB with WD 0947+452 Ref.(QL).
WD0947+857 See also (NL)(RK)
WD0948+031 See also (QJ)(NC)
WD0948+043 See also (QJ)(NC)
WD0949+256 Double degenerate ref.(JE)
WD0949+451 Resolved triple (WD+dM4.5+dM4.5) system. Ref.(MQ) See also (QP)
WD0949+484 See also (NC)
WD0949+495 See also (OK)
WD0950+021 See also (OY)(MT)
WD0950+023 See also (OK)
WD0950+139 DA star with Teff > 1E+5K, Planetary Nebula nucleus, Ref.(5P).
WD0950-200 Double degenerate close binary, Ref.(45).
WD0951+132 ZZ Ceti star Ref.(KB)
WD0951+442 See also (OY)
WD0952+094 Reclassified as carbon star; Ref.(QB)See also (NC)(MV)
WD0952+182 ZZ Ceti star Ref.(KB)
WD0953+594 See also (RF)(RS)
WD0953+621 See also (NC)
WD0954+007 DA; binary nature questionable.Ref.(QB)See also (NC)
WD0954+013 See also (OY)
WD0954+023 See also (NC)
WD0954+239 WD+MS Eclipsing Binary System. Ref.(QN).
WD0954+247 This star is listed in ref.(EE) as being a white dwarf.
WD0954+342 SW LMI is a non-radial pulsator, Ref.(44).
WD0954+697 See also (JV)
WD0954-710 See also (NL)
WD0955+017 ZZ Ceti star Ref.(KB) See also (NQ)
WD0955+247 See also (PP)(OJ)
WD0955+412 See also (NC)
WD0956+045 Visual double see A5.20 in Ref.(LJ) See also (PS)(PP)
WD0957+022 See also (PD)(MV)
WD0957+028.1 See also (NC)
WD0957+089 See also (NC)
WD0957+112 See also (NC)
WD0957-666 Possible double degenerate binary, Ref.(BY) See also (MV).
WD0958+024 See also (NC)
WD0958+102 See also (NC)
WD0959+038 See also (NC)
WD0959+441 See also (NC)
WD1000+044 See also (NC)
WD1000+220 Probably Late A or early F star Ref.(PS)
WD1000-001 See also (PP)(OK)
WD1001+058 See also (PD)(MV)
WD1001+203 Name(s) for MS companion(s). Ton1150B See also (QP)
WD1001+473 See also (NC)
WD1002+525 See also (NC)
WD1003+009 See also (QJ)(NC)
WD1003+230 WD+MS Eclipsing Binary System. Ref.(QN).
WD1003+612 See also (NC)
WD1003-441 LONGMORE 4 is a PG1159 star with 9-11 detected periods and an associated planetary nebula mass ejection, Ref.(DJ); type lgEp, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
WD1004+124 See also (NC)
WD1004+128 See also (PD)(MV)
WD1004+409 See also (NC)
WD1005+002 ZZ Ceti candidate (HC)
WD1005+465 See also (NC)
WD1006+029 See also (QJ)(NC)
WD1006+431 Superposition of three stars; Ref.(QB)
WD1007-002 See also (QJ)(NC)
WD1008+053 See also (OY)
WD1008-179 NOTE: Should be classified as an extremely hot, Teff > 100,000K, from ref(LX).
WD1009+034 See also (NC)
WD1009-184 Wide CPMB with the K7V star LHS 2231. Ref.(OJ) See also (RZ)
WD1010+043 See also (OK)
WD1010+049 See also (NC)
WD1010+049.1 See also (NC)
WD1010+064 See also (JV)(NL)(OK)
WD1011+459 See also (NC)
WD1011+470 See also (OY)
WD1011+601 ZZ Ceti star Ref.(KB) See also (NQ)
WD1012+093 See also (PD)(MV)
WD1013+033 ZZ Ceti star Ref.(KB)
WD1013+044 See also (PD)(MV)
WD1013+494 See also (NC)
WD1013-010 Single-lined double-degenerate binary. Ref.(PP)
WD1013-050 DAO white dwarf in a pre-CV, RE1016+053, REF.(BC), Quadruple system DAO + 3 dM stars, Ref(LJ) See also (QH)(MV)(RK)
WD1014+083 See also (NC)
WD1014-009 See also (QJ)
WD1015+014 Polarized magnetic white dwarf, Ref. (04) See also (PD)(MV)
WD1015+076 Finding chart for PG 1015+076B see A5.21 in Ref.(LJ)
WD1015+161 See also (QV)(QD)(QA)(PP)(OR)(MR)
WD1015+468 See also (NC)
WD1015-173 Name(s) for MS companion(s). EC 10150-1722B
WD1015-216 See also (PP)
WD1016+406 See also (NC)
WD1016+535 See also (NC)
WD1016-044 See also (QV)
WD1017+125 Finding chart for PG 1017+125B Ref.(LJ)
WD1017+366 GD116 is a magnetic degenerate, Ref.(9L).
WD1017-138 See also (PP)
WD1018+515 See also (NC)
WD1019+462 Binary (WD+M0) system. Ref.(MK) See also (PR)
WD1019+583 See also (NC)
WD1019+637 See also (OJ)
WD1020+047 See also (NC)
WD1020+442 See also (NC)
WD1020+541 See also (MS)(NR)
WD1022+009 See also (NN)
WD1022+050 Double-degenerate candidate Ref.(KP). See also (QX)
WD1022+108 See also (NC)
WD1022-301 See also (RK)(OQ)
WD1023+009 See also (PP)(OK)
WD1023+305 See also (QJ)
WD1024-002 ZZ Ceti candidate (HC)
WD1026+002 Radial Velocities 36.5/48.0 km/sec Ref.(JP) Section A3.2 in Ref.(LJ) indicates the companion is a high velocity background star, not a CPMB See also (QX)(QX)(QP)(MY)(NL)
WD1026+023 PCEB. Ref.(QH)(SM).
WD1026+117 LHS2273 is a magnetic degenerate, Ref.(28) See also (MV)
WD1026+453 See also (NL)(OK)(RK)
WD1027+398 See also (NC)
WD1027+469 See also (NC)
WD1029+537 See also (QM)(JV)
WD1030+598 See also (NC)
WD1031+063 See also (PP)
WD1031+234 A new magnetic degenerate with a field strength exceeding 500 megagauss, Ref.(9Y)(JE)N.
WD1031-114 See also (PP)(NB)(NL)(RK)
WD1032+027 See also (NC)
WD1032+109 See also (NC)
WD1032+216 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)
WD1032+393 See also (NC)
WD1032+400 Reclassified as carbon star; Ref.(QB)See also (NC)
WD1033+464 Composite spectrum with dM(GD 123B), Ref.(9V), also see Section A5.14 in Ref.(LJ) See also (QP)(NL)
WD1033+656 See also (MV)
WD1033+714 See also (OJ)
WD1034+001 Hot DO degenerate with C,N,O,Si absorption in the far UV, Ref.(AL) See also (RN)
WD1034+074 See also (RS)
WD1034+077 LHS2288 MV > 15.0, Ref.(51).
WD1034+492 See also (OK)
WD1034+661 See also (NC)
WD1036+021 Peculiar secondary star. Ref.(QB)
WD1036+085 See also (OK)
WD1036-204 LP790-29 is a polarized,carbon band,magnetic degenerate, Ref.(5G) See also (PS)(OJ).
WD1037+256 See also (QJ)
WD1037+512 Name(s) for MS companion(s). PG 1037+512B
WD1037+521 See also (NC)
WD1038+088 See also (QJ)(NC)
WD1038+096 See also (NC)
WD1038+518 See also (NC)
WD1038+633 See also (OK)
WD1039+447 See also (NC)
WD1040+054 See also (NC)
WD1040+406 See also (NC)
WD1040+421 See also (OY)
WD1040+451 See also (JV)(OK)
WD1040+492 See also (QM)
WD1041+063 See also (QJ)(NC)
WD1041+091 See also (QD)(OR)
WD1041+580 See also (QP)(NL)(NO)
WD1042+322 See also (PE)
WD1042-000 See also (QJ)(NC)
WD1042-690 PCEB DAQZ + dM5 Ref.(RV).See also (QH)(PP)(MV)
WD1043+600 See also (NC)
WD1043+610 See also (NC)
WD1043-034 CPMB system with the F9 V star G163-B9A. Ref.(OF)
WD1043-188 See also (OJ)(NN)(PR)
WD1045+056 PCEB Ref.(QH).See also (QJ)(NC)
WD1045+629 See also (NC)
WD1045-091 HE1045-0908:a new magnetic DA white dwarf with a distinctive Zeeman line splitting pattern, Ref.(8R).
WD1046+398 See also (NC)
WD1047-046 See also (QX)
WD1048+668 See also (NC)
WD1049+103 Name(s) for MS companion(s). PG 1049+103B
WD1049+266 See also (QJ)
WD1050+522 Double-degenerate merger system. Ref.(QT).See also (QS)(SL)
WD1050+541 Reclassified as M star; Ref.(QB)See also (NC)
WD1050+598 See also (PD)(MV)
WD1051+516 Name(s) for MS companion(s). SBS 1051+516B See also (QP)
WD1051+533.1 CPMB with WD1051+533.2
WD1051+533.2 CPMB with WD1051+533.1
WD1052+273 See also (QP)(MY)(NL)
WD1053+001 ZZ Ceti star Ref.(KB)
WD1053+017 See also (RF)(RS)
WD1053+049 See also (NC)
WD1053+511 See also (NC)
WD1053+656 See also (PD)(MV)
WD1053-092 See also (PP)
WD1053-290 See also (PP)
WD1053-550 Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart See also (MV)
WD1054+501 Reclassified as M star; Ref.(QB)
WD1055-072 DA6 observed to be featureless? Ref.(9V)(NB)(NN) See also (PV)(PO)(OL)(OJ)(RQ).
WD1056+012 See also (NC)
WD1056+516 DA1 may be a double degenerate, Ref.(81)(JV) See also (OK)(RK)
WD1056+559 See also (OY)
WD1056-384 See also (PP)(RK)
WD1057+719 See also (QP)(NL)(RK)
WD1058+078 See also (NC)
WD1058+140 See also (QJ)
WD1058-129 See also (PP)
WD1059+126 See also (QJ)(NC)
WD1059+559 Relcassified as M star + bright star nearby; Ref.(QB)
WD1101+364 double degenerate DA + DA double lined, Ref.(7F). See also (QX)
WD1102+095 Single-lined double-degenerate binary. Ref.(PP)
WD1102+253 Detached magnetic cataclysmic variable. Ref.(QB)
WD1102+748 See also (MY)
WD1102-183 See also (QA)(PP)(OH)
WD1103+015 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1103+078 See also (NC)
WD1103-008 See also (NC)
WD1104+602 See also (QP)(NL)
WD1104+656 See also (NC)
WD1105+053 See also (NC)
WD1105+097 See also (NC)
WD1105+412 See also (PR)
WD1105-048 See also (JE)(MZ)(NL)(PR)
WD1105-340 CPMB with M4Ve companion Ref.(MD)
WD1106+121 See also (NC)
WD1106+316 Name(s) for MS companion(s). Ton 058B
WD1107+055 Reclassified as MS+galaxy; Ref(.QB)See also (NC)
WD1107+310 Wide-binary? Ref.(QB)
WD1107+602 See also (PD)(MV)
WD1107-257 Common proper motion pair. See also (PR)
WD1108+207 See also (NN)
WD1108+325 Name(s) for MS companion(s). Ton 060B See also (QP)
WD1108+563 See also (OK)
WD1109+244 See also (JV)(NL)
WD1109-005 ZZ Ceti candidate (HC)
WD1111+455 See also (NC)
WD1112+096 See also (QJ)(NC)
WD1112+432 Reclassified as CV; Ref. QB)
WD1112+669 See also (NC)
WD1113+542 See also (NC)
WD1114+026 See also (NC)
WD1114+113 See also (QJ)(NC)
WD1115+017 See also (QJ)(NC)
WD1115+101 See also (PD)(MV)
WD1115+135 See also (QJ)(NC)
WD1115+158 A new pulsating DB star, Ref.(DV).
WD1115+166 An Unresolved DAB Double Degenerate Binary. (GW)(HE)(JE)N See also (QX)(QX)
WD1116+026 ZZ Ceti (OD)See also (QV)(QD)(QA)(PP)(OR)(MR)(NL)
WD1116+301 See also (QX)
WD1116-470 See also (PV)
WD1119+042 ZZ Ceti star Ref.(KB)
WD1120+008 See also (QJ)(NC)
WD1120+102 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)
WD1120+439 See also (MY)
WD1120+509 Spectrum shows Mg I, Ref.(JJ)
WD1121+216 Ross 627 is a DA white dwarf not DA, F or DF, Ref.(6A) See also (PV)(PO)(OL)(MM)(NB)(NN)(OJ)(RQ)
WD1121-008 See also (NC)
WD1122+546 See also (OK)
WD1123+014 See also (QJ)(NC)
WD1123+040 ZZ Ceti star Ref.(KB) See also (NQ)
WD1123+056 MS+MS superposition Ref.(QB)
WD1123+189 Composite DA + DM binary, Ref.(9V) See also (QP)(MY)(NL)
WD1124+152 See also (QJ)
WD1124+431 See also (NC)
WD1124-018 Single-lined double-degenerate binary. Ref.(PP)
WD1124-293 See also (QV)(QA)(OH)
WD1125+131 See also (NC)
WD1125-002 See also (QJ)(NC)
WD1126+089 See also (NC)
WD1126+185 See section A1.3 in Ref. (LJ).
WD1126+499 NOTE: 2000 coords are from ref(MH),Ref(LR) gives J112924.74+493931.9 but no star found at these coords using SDSS Finding Chart Tool. See also (PD)(MV)
WD1126+668 See also (QJ)(NC)
WD1126-008 See also (PD)(MV)
WD1127+319 See also (PE)
WD1129+071 See also (PP)
WD1129+284 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)
WD1129-030 See also (QJ)(NC)
WD1131+521 See also (PD)(MV)
WD1132+661 See also (QJ)(NC)
WD1132-298 (P.Bergeron Finding Chart)
WD1132-325 Sirius-like system. Ref.(RZ) See also (OJ)
WD1133+358 Name(s) for MS companion(s). G147-065B
WD1133+489 Name(s) for MS companion(s). PG1133+489B See also (QP)
WD1134+044 See also (QJ)(NC)
WD1134+300 No 1400a absorption feature observed, Ref.(CL)(JV) See also (QP)(MY)(NB)(NL)(OJ)
WD1135+000 See also (NC)
WD1135+579 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) See also (MV)
WD1136+514 See also (NC)
WD1136-015 LBQS1136-0132 is a magnetic degenerate, Ref.(85) See also (PD)(MV)
WD1137+423 ZZ Ceti star ref.(KA) See also (RY)
WD1137+582 Reclassified as M star + bright star nearby; Ref.(QB)
WD1137+614 See also (MV)
WD1138+046 See also (NC)
WD1138-026 See also (NC)
WD1140+004 ZZ Ceti candidate (HC) PCEB. Ref.(QH). See also (QP)(QJ)(PS)(NC)
WD1141+462 See also (NC)
WD1141+504 See also (NC)
WD1142+385 Cataclysmic variable? Ref.(QB)
WD1142-645 L0145-141 shows strong UV absorption features, Ref.(DC) Member of binary or multiple star system. Ref.(OJ) See also (PC)(OE).
WD1143+321 See also (QP)(NL)(1P)(AP)
WD1144+004 PG1159 degenerate, Ref.(DI); type EP, Ref.(66)(JV) See also (RN)
WD1144+016 MS+MS superposition; Ref.(QB)
WD1144+299 See also (PE)
WD1144-246 See also (PP)
WD1145+041 See also (QJ)(NC)
WD1145+187 See also (QP)(PP)
WD1145+487 See also (PD)(MV)
WD1146+443 See also (NC)
WD1146-015 See also (NC)
WD1147+255 Common proper motion binary Ref.(JP) See also (PP)(PQ)(PR)
WD1147-010 See also (NC)
WD1148+544 LP129-587 is a CPMB with LP129-586 Ref.(JL) See also (OK)
WD1148-230 = EC11481-2303 See also (NF)
WD1149+001 Irradiated secondary star. Ref.(QB)See also (QJ)(NC)
WD1149+057 ZZ Ceti (OC) See also (PP)
WD1149+280 See also (PE)
WD1150+006 See also (NC)
WD1150-153 Short period ZZ Ceti (OC) See also (QD)(QA)(OR)
WD1151+015 See also (PD)(MV)
WD1151+548 See also (NC)
WD1151-029 PG1159 degenerate, Ref.(DN); type LGE, Ref.(66).
WD1152-000 See also (RS)
WD1154+061 ZZ Ceti star Ref.(KB)
WD1154+456 DB; binary nature questionable. Ref.(QB) See also (QM)
WD1155+492 See also (QX)
WD1156+117 See also (NC)
WD1156+129 Name(s) for MS companion(s). WD 1156+129B
WD1156+132 See also (PS)
WD1156+619 See also (PD)(MV)
WD1158-362 See also (RK)
WD1159+619 See also (PD)(MV)
WD1159+803 G255-002 is a ZZ CETI variable, Ref.(BN). See also (PB)
WD1159-034 Proto-type of a new class of pulsating, hot, helium-rich DO degenerates (PG1159), Ref.(7K); type E, Ref.(66)(JV) Non-radial g-mode pulsator Ref.(KO) See also (RN)
WD1200+548 See also (OK)
WD1201+035 See also (QJ)(NC)
WD1201-001 See also (PP)(MZ)
WD1201-023 ZZ Ceti candidate (HC)
WD1202+034 See also (QJ)(NC)
WD1202+608 Peculiar DAO white dwarf in a pre-CV; binary? Ref.(29), close double degenerate Ref.(3L)(JE)N. See also (QX)
WD1202-232 See also (QV)(PP)(OJ)(OL)(RQ)
WD1203+085 See also (PD)(MV)
WD1203+097 See also (NC)
WD1203+432 See also (QJ)(NC)
WD1204+444 See also (PD)(MV)
WD1204+450 Triple system Finding chart for PG 1204+450C see A5.5 in Ref.(LJ)
WD1204-026 ZZ Ceti candidate (HC)
WD1204-136 See also (QA)(OH)
WD1206+654 See also (NC)
WD1207-005 See also (QJ)(NC)
WD1207-157 See also (PP)
WD1208+039 See also (NC)
WD1208+422 See also (NC)
WD1208+576 See also (OJ)(OH)
WD1208-025 See also (QJ)(NC)
WD1209+018 Magnetic DA+L brown dwarf; Ref.(QB)See also (PD)(NC)(MV)
WD1210+140 Single-lined double-degenerate binary. Ref.(PP) See also (QP)
WD1210+464 Name(s) for MS companion(s). PG 1210+464B See also (QP)
WD1210+533 Peculiar DAO white dwarf, Ref.(3M)(JE),Spectroscopic Variable,Ref(QM).
WD1210-011 WD/MS eclipsing binary system. Ref.(PH) PCEB(SD) See also (NC)(QH)(QN)
WD1210-060 CMPB with the K3V star HIP 59519. Ref.(SH)
WD1211+332 See also (QP)
WD1211+392 See also (PR)
WD1211-025 MS+MS superposition; Ref.(QB)See also (NC)
WD1211-169 HS1211-170 is a new magnetic degenerate, Ref.(4C).
WD1212+369 See also (QH)
WD1212+589 See also (NC)
WD1212-022 Heavily blanketed, cool(~6000K) magnetic(Zeeman split NaI and MgI) DZ. (EM)
WD1213+096 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1213+437 See also (NC)
WD1213+528 DA and dwarf M spectroscopic binary post-common envelope, Ref.(5A); DA degenerate with T=13,000K; log g=8; 1400A absorption, Ref.(AQ)(JV). See also (QX)(SM)
WD1213+532 DA; binary nature questionable. Ref.(QB) See also (QM)
WD1214+032 Companion = LP554-064 with Vmag=13.28 See also (PR)
WD1214+267 See also (JE)
WD1214-001 See also (PD)
WD1215+009 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1215+024 See also (OK)
WD1215+323 See also (PR)
WD1216+036 See also (PP)
WD1217+475 DC; binary nature questionable. Ref.(QB)
WD1217+635 See also (NC)
WD1218+496 See also (NC)
WD1218+497 Name(s) for MS companion(s). PG 1218+497B See also (QP)
WD1219+005 See also (PD)(MV)
WD1219+098 See also (NC)
WD1219-024 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1220+234 PG1220+234 is a magnetic degenerate, Ref.(31) See also (MV)
WD1220+441 See also (OY)
WD1220+484 See also (PD)(MV)
WD1220-003 See also (OY)
WD1221+422 See also (PD)(MV)
WD1221-006 See also (QJ)(NC)
WD1223-659 See also (OJ)(MM)(OL)(RQ) (P.Bergeron Finding Chart)
WD1224+309 PCEP(QH) See also (QJ)
WD1225+006 See also (QV)(QA)
WD1225+589 DA; binary nature questionable.Ref.(QB) See also (QM)
WD1225+637 Spectrum shows Mg I, Ref.(JJ)
WD1225-015 See also (NC)
WD1225-079 See also (PS)(OR)
WD1226+109 See also (QD)(QA)(OR)
WD1227+292 See also (PR)
WD1228+541 See also (NC)
WD1229+290 See also (JV)
WD1229+558 See also (QJ)(NC)
WD1229-028 See also (QJ)(NC)
WD1230+163 Double-degenerate merger system. Ref.(QT).
WD1230+596 See also (NC)
WD1230+605 See also (NC)
WD1231+130 DA; binary nature questionable.Ref.(QB)See also (PD)(NC)(MV)
WD1231+447 See also (NC)
WD1231-021 Double-degenerate merger system. Ref.(QT).
WD1232+065 See also (QJ)
WD1234+481 Hot DA and a very low-mass detached companion. Ref.(RO).See also (QP)(JV)(NB)(NL)(SM)
WD1235+012 DA; binary nature questionable.Ref.(QB)See also (NC)
WD1235+294 Coordinates in ref (BV) are incorrect, Private Communication 4/24/2011 P.Bergeron
WD1235+620 See also (NC)
WD1236+012 See also (NC)
WD1236+457 Listed in ref (NN) as WD1239+454
WD1236+661 See also (NC)
WD1236-004 Name(s) for MS companion(s). WD 1236-004B See also (QP)
WD1236-495 BPM 37093 is a ZZ CETI variable, Ref.(44) See also (PP)(PB)(MY)(NB)(NL)(OJ)
WD1237+487 See also (NC)
WD1237-028 See also (MY)
WD1238+439 See also (NC)
WD1238+618 See also (NC)
WD1239+143 See also (QJ)
WD1239+277 See also (RY)
WD1240+453 See also (NC)
WD1240+644 See also (NC)
WD1241+151 See also (QJ)
WD1241+235 See also (PP)
WD1241+483 See also (OK)
WD1241-010 New double degenerate close binary, Ref.(7G), Triple system, see section A5.6 in Ref.(LJ). See also (QX)(PP)(RO)
WD1242+105 WD+MS Eclipsing Binary System. Ref.(QN).
WD1242-105 See also (OJ)
WD1244+149 See also (PQ)
WD1244+498 See also (RS)
WD1244-125 See also (PP)
WD1245+413 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)See also (MV)
WD1246+441 See also (NC)
WD1246-022 See also (PD)(MV)
WD1247+042 See also (PE)
WD1247+381 See also (QJ)
WD1247+550 Possibly the coolest known degenerate star, Ref.(5S)See Also(5N)(MQ)(NN)(OK).
WD1247-176 Name for MS companion EC 12477-1738B, PCEB(QH)
WD1248+009 See also (NC)
WD1248+161 See also (PD)(MV)
WD1248-610 (P.Bergeron Finding Chart)
WD1249+016 See also (QJ)(NC)
WD1249+044 ZZ Ceti (OC)
WD1249+160 See also (OK)
WD1249+182 See also (PP)
WD1249+450 See also (NC)
WD1250-018 See also (QJ)(NC)
WD1250-226 The central star of the Planetary Nebula A3, is a binary consisting of a white dwarf and a cool G8 IV star.(HD)
WD1251+561 Reclassified as M star + nearby bright star; Ref.(QB)
WD1251+584 See also (NC)
WD1252+031 See also (NC)
WD1252+559 MS+MS superposition; Ref. QB)See also (NC)
WD1252+564 See also (PD)(MV)
WD1253+024 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1253+261 Central Star of PN LoTr 5, Ref.(JV) See also (SM)
WD1253+378 HZ 34 is classified DAO in Ref.(DN)(JE)N.
WD1253+385 Reclassified as M star; Ref.(QB)
WD1254+003 ZZ Ceti candidate (HC)
WD1254+019 See also (QJ)(NC)
WD1254+223 See also (PP)(PM)(JV)(NL)(RK)(SM)
WD1254+345 HS1254+3430 is a magnetic degenerate, Ref.(63).
WD1254+428 See also (NC)
WD1255+431 See also (RS)
WD1255+481 See also (NC)
WD1255+552 See also (NC)
WD1255-019 See also (OY)
WD1257+037 See also (OJ)(NN)
WD1257+047 Finding chart for GD 267B Ref.(LJ) See also (PP)
WD1257+278 See also (QA)(MY)(RT)(RY)
WD1257-723 (P.Bergeron Finding Chart)
WD1258+013 ZZ Ceti star Ref.(KA) NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog. See also (OK)
WD1258+593 Finding chart for GD 322B Ref.(LJ)
WD1259+053 See also (QJ)(NC)
WD1300+062 Reclassified as M star; Ref.(QB)
WD1300+263 See also (NN)
WD1300-005 See also (OK)
WD1302+412 See also (OY)
WD1302+597 GD323 is classified DAB (peculiar). First known stratified H/HE atmosphere? Ref.(5W)(4K). See also (QM)
WD1304+227 Common proper motion pair. See also (NZ)(PR)
WD1305+125 See also (NC)
WD1305+627 See also (OY)
WD1305-017 See also (OK)
WD1307+354 GD 154 is a ZZ CETI variable, Ref.(8Y) See also (PB)(PA)(NL)
WD1307-017 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1307-141 Name(s) for MS companion(s). EC 13077-1411B
WD1308+537 See also (NC)
WD1309+853 A new magnetic degenerate with a 4.9 Mg field (8N) See also (MV)(OJ)
WD1310+583 See also (OJ)
WD1310+597 See also (NC)
WD1310-230 An interacting double-degenerate binary star with a period of 65.1 min. (FL) See also (SM)
WD1310-472 A new, very low luminosity, degenerate star, one of the intrinsically faintest white dwarfs known, Ref.(9E) See also (OJ).
WD1311+028 See also (QJ)(NC)
WD1312+098 PG1312+098 is a magnetic degenerate, Ref.(9Z).
WD1312+156 See also (NC)
WD1314+003 See also (MS)(NR)
WD1314+293 HZ43 soft X-ray EUV source, Ref.(7C) See also (QP)(QM)(JV)(NL)(OK)(PR)(RK)(SM)
WD1314-153 The star indicated in both the Marsh and Arizona finding charts is at 13 16 47.5 -15 36 05 This is not consistent with the coords above which are for LP737-047, LHS2712 and NLTT33503. Also the coordinates on the Marsh chart are not consiste
WD1315-110 See also (QV)(QA)
WD1315-781 See also (OJ)
WD1317+018 See also (QJ)(NC)
WD1317+117 See also (NC)
WD1317+135 See also (PD)(MV)
WD1317+453 Newly identified double degenerate close binary, Ref.(7G)(JV). See also (QX)
WD1318+042 See also (NC)
WD1318+664 See also (NC)
WD1319+019 See also (QJ)
WD1320+645 See also (OK)
WD1320-026 See also (NC)
WD1321+083 See also (QJ)
WD1321+305 See also (PE)
WD1321+545.1 See also (NC)
WD1322+130 See also (NC)
WD1323+656 See also (RS)
WD1323-514 (P.Bergeron Finding Chart)
WD1324+004 See also (QJ)(NC)
WD1324+458 WD/MS eclipsing binary system. Ref.(PH) See also (QX)(QH)
WD1324+458.1 See also (PH)
WD1325+581 See also (JV)
WD1326+120 See also (QJ)(NC)
WD1326+127 WD+MS Eclipsing Binary System. Ref.(QN).
WD1326+132 See also (QJ)(NC)
WD1327+594 See also (MV)
WD1327-083 1400a absorption feature, Ref.(CL). See also (KP)(NB)(NL)(OJ)
WD1328+017 See also (NC)
WD1328+089 See also (QJ)
WD1328+307 G165-007 has more identifiable line features than any other known degenerate, Ref.(DA)(QA).
WD1328+461 See also (NC)
WD1328+648 Spectrum shows Na I, Ref.(JJ)
WD1329+666 See also (NC)
WD1330+015 G62-46 is an unresolved double degenerate with a magnetic DA and a DC white dwarf, Ref.(24) See also (PS)(MV)
WD1330+643 See also (OY)
WD1331+111 See also (NC)
WD1332+643 See also (PD)(MV)
WD1333+005 MS companion=LP618-014B Eclipsing Binary System. Ref.(QN) See also (QP)
WD1333+130 See also (QJ)
WD1333+152 See also (QJ)
WD1333+487 Spectroscopic composite DB + DM, Ref.(1V),Triple-star system: DB3.2+dM4+dM6.5 Ref.(QO). See also (QP)
WD1333+510 See also (JV)
WD1333-012 See also (NC)
WD1334+013 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1334+039 See also (OJ)(NN)
WD1334+070 Single-lined double-degenerate binary. Ref.(PP)
WD1334-001 See also (OW)
WD1334-001.1 See also (NC)
WD1334-160 See also (PP)(MY)(PQ)(PR)
WD1334-326 PCEB. Ref.(QH) MS companion=EC 13349-3237B
WD1334-678 (P.Bergeron Finding Chart)
WD1335+001 ZZ Ceti candidate (HC)
WD1335-001 See also (PY)
WD1336+123 Common proper motion pair. See also (PR)
WD1336+422 See also (NC)
WD1337+021 See also (QJ)(NC)
WD1337+598 See also (NC)
WD1337+705 See also (QA)(NL)(OK)
WD1339+050 See also (QJ)(NC)
WD1339+346 See also (PS)
WD1339+606 Name(s) for MS companion(s). SBS 1339+606B See also (QP)
WD1339+616 See also (NC)
WD1339+659 See also (PD)(MV)
WD1339-340 VR = 212 km/sec corrected for gravitational redshift ref.(MI)
WD1341+036 See also (PM)
WD1341+056 See also (QJ)
WD1342+414 See also (NC)
WD1342+443 Single WD model atmosphere does not fit balmer lines, Ref.(81) See also (OK).
WD1342+672 See also (MS)(NR)
WD1343-006 ZZ Ceti star Ref.(KB)
WD1344+090 See also (QJ)
WD1344+106 See also (QA)(OJ)(NN)(OH)
WD1344+572 See also (QP)
WD1345+238 Common proper motion binary Ref.(JP) See also (PF)(OJ)(NN)(PR)
WD1345+417 See also (NC)
WD1346+188 WD+MS Eclipsing Binary System. Ref.(QN) See also (QH)
WD1347+029 See also (RS)
WD1347+477 See also (NC)
WD1347-129 Eclipsing binary (EH) See also (PP)(SM)
WD1348+400 DA; binary nature questionable. (Ref.(QB)See also (NC)
WD1348+442 See also (OK)
WD1348-273 See also (PR)
WD1349+144 Double-lined double-degenerate binary. Ref.(PP)See also (JE)
WD1349+545 SBS1349+5434 is a magnetic degenerate, Ref.(5T). See also (PD)
WD1349+552 ZZ Ceti star ref.(KA)(OC) See also (PB)(OK)
WD1349-230 See also (OR)
WD1350+457 See also (NC)
WD1350+656 ZZ CETI variable, Ref.(87)(JE)N. See also (PB)(NQ)(OK)
WD1350-090 WD1350-090 is a magnetic degenerate, Ref.(9W) See also (OJ).
WD1351+489 A new pulsating DB star, Ref.(DV).
WD1352+004 See also (OR)
WD1352+013 ZZ Ceti star Ref.(KB)
WD1352+421 Irradiated secondary star. Ref.(QB)
WD1352-022 See also (NC)
WD1353+409 See also (RL)
WD1354+340 CPMB WITH BD+34 2473 See also (NZ)(PQ)
WD1357+366 See also (NC)
WD1359+256 See also (QJ)
WD1400+005 See also (OK)
WD1401+005 Conflicting locations - Aladin image is centered on Marsh's ID while Arizona ID is the blue star directly to the right of center.
WD1401+051 See also (MS)
WD1401+438 See also (SM)
WD1401-014 See also (NC)
WD1401-147 ZZ Ceti star ref.(KA)
WD1402+545 See also (NC)
WD1403+043 See also (NC)
WD1403+451 See also (NC)
WD1403-077 See also (PP)(JV)
WD1404+008 See also (NC)
WD1404+603 See also (QJ)(NC)
WD1405+008 See also (OY)
WD1406+050 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
WD1407+425 See also (QA)(OK)
WD1407-023 See also (RF)(RS)
WD1407-475 Variability in radial velocity indicates a possible binary with a period of ~ 1 day. (EE) (P.Bergeron Finding Chart)
WD1408+323 See also (QP)(QC)
WD1408-018 WD+MS Eclipsing Binary System. Ref.(QN) See also (NC)
WD1409+107 PCEB. Ref.(QH).
WD1409+233 WD+MS Eclipsing Binary System. Ref.(QN).
WD1410+051 See also (OY)
WD1410+168 See also (PP)
WD1410+269 See also (QJ)
WD1411+659 See also (PE)(NC)
WD1412+612 New magnetic degenerate, Ref.(63).
WD1412-013 PCEB. Ref.(QH) See also (QJ)(NC)
WD1412-049 Name(s) for MS companion(s). PG 1412-049B
WD1413+015 WD/MS eclipsing binary system. Ref.(PH) See also (QH)(NL)(QN)
WD1413+241 See also (RY)
WD1414+012 ZZ Ceti star Ref.(KB)
WD1414+020 See also (QJ)(NC)
WD1414+350 See also (PE)
WD1414-088 Component B of the double-lined DA+DA binary system HE 1414-0848. (HG)
WD1414-088.1 Component A of the double-lined DA+DA binary system HE 1414-0848. (HG)
WD1415+132 See also (QJ)
WD1416+060 binary nature questionable.Ref.(QB)
WD1416+077 See also (QJ)
WD1416+259 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)
WD1416+633 Binary (WD+dM) system. Ref.(MK)
WD1416+644 See also (PR)
WD1417+473 See also (QJ)(NC)
WD1418-088 Double degenerate system. Ref.(JP)
WD1419+252 Has an Unresolved companion DA5.0 White Dwarf with (Vmag = 18.10 AbsMag = 12.14) Ref(QC)
WD1419+576 Resolved triple (WD+dM2+dM2) system. Ref.(MQ) See also (QP)
WD1420+441 Possible double-degenerate system. Ref.(QS).
WD1420+518 See also (NC)
WD1421+243 WD/MS eclipsing binary system. Ref.(PH) See also (QN)
WD1421+527 See also (RS)
WD1422+095 CX BOO is a ZZ CETI variable, Ref.(44). See also (PP)(PB)(SF)
WD1422+497 See also (NC)
WD1423+027 See also (QJ)(NC)
WD1423+371 See also (NC)
WD1424+534 PG1159 DO degenerate, Ref.(DN); type A, Ref.(66).
WD1424+602 See also (NC)
WD1425+375 See also (PD)(MV)
WD1425+540 G200-39 common proper motion binary with G200-40 (K dwarf). Prototype of the class of DBA stars, Ref.(5R).
WD1425-811 L0019-002 is a ZZ CETI variable, Ref.(7I) See also (PP)(PB)(8Z)(NB)(NL)(OD)
WD1426-276 See also (PP)
WD1427-024 See also (QJ)(NC)
WD1428+114 See also (QJ)
WD1428+373 Double-degenerate system. Ref.(QX) See also (PS)(OK)
WD1428+582 PCEB. Ref.(QH).
WD1429-037 ZZ Ceti (OC)
WD1429-121 Non-radial g-mode pulsator Ref.(KO)
WD1430+041 See also (RS)
WD1430+070 See also (QJ)
WD1430+432 See also (PD)(MV)
WD1430+460 See also (PD)(MV)
WD1431+614 See also (NC)
WD1432-164 PCEB. Ref.(QH).
WD1433+367 See also (QJ)(NC)
WD1433+377 WD/MS eclipsing binary system. Ref.(PH) See also (QJ)(NC)(QH)
WD1433+538 See section A5.15 in Ref. (LJ)MS companion=GD 337B See also (QJ)(QH)(PE)(NC)
WD1434+289 See also (PS)
WD1434+503 Double-degenerate merger system. Ref.(QT)(SL).
WD1435+370 Name(s) for MS companion(s). CBS194B
WD1435+383 See also (QJ)(NC)
WD1435+433 DA; binary nature questionable.Ref.(QB)
WD1435+621 See also (NC)
WD1436+424 See also (NC)
WD1436+526 See also (OK)
WD1436+578 See also (NC)
WD1436-216 Name(s) for MS companion(s). EC 14363-2137B
WD1437+102 Possible double-degenerate system. Ref.(QS).
WD1437+368 See also (NC)
WD1437+417 See also (QJ)
WD1437-008 See also (QJ)(NC)
WD1440+003 See also (QJ)(NC)
WD1440+017 ZZ Ceti star Ref.(KB)
WD1440+753 See also (OQ)(MV)(NO)(RK)
WD1441-007 See also (OK)
WD1443+336 Name(s) for MS companion(s). PG 1443+336B See also (QP)
WD1443+414 DA; binary nature questionable.Ref.(QB)
WD1443+590 See also (RS)
WD1444+102 See also (QJ)
WD1444+592 See also (PD)(MV)
WD1444+636 See also (QM)
WD1444+636 See also (JV)
WD1444-174 See also (OJ)(NN)
WD1445+414 See also (NC)
WD1446+050 DA; binary nature questionable.Ref.(QB)See also (NC)
WD1446+575 See also (MS)(NR)
WD1447+356 See also (QJ)(NC)
WD1447-190 Reported as sdB in an earlier Ref. (EH).
WD1448+077 See also (PP)
WD1448+419 See also (QJ)(NC)
WD1449+003 G066-036 common proper motion binary with G66-35 (G5 dwarf), Ref.(75). SectionA2.2 in Ref.(LJ) reports different motions for the pair therfore not CPMB. See also (PQ)
WD1449+168 Finding chart for PG 1449+168B Ref.(LJ) See also (PP)
WD1449+522 DA binary nature questionable.(faint star nearby); Ref.(QB)See also (NC)
WD1449+559 See also (QJ)(NC)
WD1450+011 See also (QJ)(PE)(NC)
WD1451+006 NOTE: Simbad currently shows coordinates for WD1451+006.1 not WD1451+006 See also (PP)(MZ)
WD1451+006.1 Mistakenly identified as WD1451+006 in Ref. (MH) See also (OK)
WD1451+411 See also (QJ)(NC)
WD1452+435 See also (PD)(MV)
WD1452+553 See also (OK)
WD1452-022 See also (NC)
WD1454+163 WD+MS Eclipsing Binary System. Ref.(QN).
WD1454+486 See also (NC)
WD1454+595 See also (QJ)(NC)
WD1454+614 See also (NC)
WD1454-630.1 L151-81 a rare binary with DA and DB components, Ref.(8A).
WD1454-630.2 L151-81 a rare binary with DA and DB components, Ref.(8A).
WD1455+298 Possible binary (OH) See also (QA)(PS)(OR)
WD1456+103 CW BOO is a non-radial pulsator, Ref.(44).
WD1456+106 See also (QJ)
WD1456+475 See also (RS)
WD1456+515 DA; binary nature questionable.Ref.(QB) See also (NC)
WD1457+349 See also (QJ)(NC)
WD1457+455 DA; binary nature questionable.Ref.(QB) See also (NC)
WD1457+462 DA; binary nature questionable.Ref.(QB) See also (NC)
WD1457-086 See also (QV)(QD)(QA)(PP)
WD1458+045 See also (NC)
WD1458+171 Name(s) for MS companion(s). PG 1458+171B See also (QP)
WD1459+001 ZZ Ceti star Ref.(KB) NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog.
WD1459+013 See also (PJ)(NC)
WD1459+333 See also (OK)
WD1459+347 See also (MY)(OK)
WD1500+011 See also (NC)
WD1500+447 See also (NC)
WD1500-170 See also (PP)
WD1501+664 H1504 may be the hottest known star,H and He lines absent;high gravity OVI features; HEAO-1 A-2 and EXOSAT powerful soft X-ray source, Ref.(7X); type EP, Ref.(66)(JV)(KL).
WD1502+324 See also (QJ)(NC)
WD1502+349 Name(s) for MS companion(s). CBS223B
WD1502+586 See also (NC)
WD1503+331 DA + some red excess; Ref.(QB)See also (NC)
WD1503-070 See also (MV)
WD1503-093 See also (PP)
WD1504+006 See also (QJ)(NC)
WD1504+546 Name(s) for MS companion(s). CBS301B See also (QP)
WD1504-011 PCEB. Ref.(QH) See also (QJ)(NC)
WD1504-770 (P.Bergeron Finding Chart)
WD1505+483 See also (NC)
WD1506+399 See also (PD)(MV)
WD1506-019 DA; binary nature questionable.Ref.(QB)
WD1507+021 See also (PP)
WD1507+434.1 See also (NC)
WD1507-105 See also (PP)
WD1508+008 See also (QJ)(NC)
WD1508+025 See also (QJ)(NC)
WD1508+409 See also (QJ)(NC)
WD1509+020 See also (QJ)(NC)
WD1509+322 See also (NB)
WD1509+425.1 See also (MV)
WD1510+566 See also (OK)(PR)
WD1511+009 See also (PP)(OK)
WD1511-048 Single-lined double-degenerate binary. Ref.(PP)
WD1514+353 See also (NC)
WD1514+411 See also (PR)
WD1516+348 DA; binary nature questionable.Ref.(QB)
WD1516+460 See also (QJ)(NC)
WD1516+534 See also (NC)
WD1516+612 See also (PD)(MV)
WD1517+502 A rare dwarf carbon star plus white dwarf binary, Ref.(5I),(MQ)Reclassified as carbon star; Ref.(QB) See also (NC)
WD1517+740 HS1517+7403 is a PG1159 star with no detected variability, Ref.(DI); type A, Ref.(66).
WD1518+328 See also (QJ)(NC)
WD1518+381 DB; binary nature questionable.Ref.(QB)See also (NC)
WD1519+323 See also (NC)
WD1519+422 See also (QJ)
WD1519+500 See also (OK)
WD1519+611 See also (NC)
WD1520+388 See also (NC)
WD1520+525 PG1520+535 is a PG1159 star with a detected planetary nebula but no detected variability, Ref.(DI) DO degenerate, Ref.(DN).
WD1521+310 See also (JE)
WD1521+352 DA; binary nature questionable.Ref.(QB)
WD1521-003 ZZ Ceti star Ref.(KB)
WD1522+462 See also (QJ)(NC)
WD1522+479 See also (NC)
WD1522+508 Name for MS companion CBS318B See also (QP)(QH)
WD1522+662 See also (JV)
WD1524+005.1 See also (NC)
WD1524-749 (P.Bergeron Finding Chart) See also (PP)
WD1526+005 PCEB Ref(QH) See also (QJ)(NC)
WD1526+013 See also (OK)
WD1526+333 See also (NC)
WD1526+348 See also (QJ)(NC)
WD1528+087 Post-common envelope binary. Ref.(QB)
WD1528+487 See also (QM)
WD1529+141 See also (OJ)
WD1529-772 See also (MV)(RK)
WD1530+037 See also (NC)
WD1530+315 Reclassified as M star + nearby bright star; Ref.(QB)
WD1530-019 NOTE: 2000 coords are from ref(MH),Ref(LU) gives J153332.9-020600.0 but no star found at these coords using SDSS Finding Chart Tool.
WD1531+746 ZZ Ceti (OC)
WD1531-022 See also (MY)
WD1532+033 See also (NL)
WD1532+394 See also (QJ)(NC)
WD1532+415 See also (QJ)(NC)
WD1532+420 See also (NC)
WD1533+423 See also (PD)(MV)
WD1533-057 New magnetic degenerate, Ref.(5U)(JE)N.
WD1534+503 Double degenerate system? Radial velocities -106/159? Ref.(JP) See also (OK)
WD1537+382 See also (NC)
WD1537+532 See also (PD)(MV)
WD1537+651 See also (JE)
WD1537-006 DA; binary nature questionable.(Ref. QB)See also (NC)
WD1537-152 See also (PP)
WD1538+333 See also (OJ)
WD1539+035 See also (QJ)(NC)
WD1539+039 See also (PD)(MV)
WD1539+333 See also (NC)
WD1539+530 Finding chart for PG 1539+530B see A5.11 in Ref.(LJ)
WD1541+061 See also (NC)
WD1541+297 DA; binary nature questionable.(Ref. QB)
WD1541+558 See also (NC)
WD1541+650 ZZ Ceti star ref.(JE)(OC)
WD1541-381 See also (PP)(SM)
WD1542+182 See also (QD)
WD1542+392 Reclassified as M star; Ref.(QB)
WD1542-275 Common proper motion pair. See also (PR)
WD1543+332 See also (NC)
WD1544+009 CPMB system with the G0 star BD+01 3129. Ref.(OF)(PR)
WD1544+218 See also (QJ)
WD1544-377 L481-60 common proper motion binary with HR5965 (G6 dwarf) See also (PP)(OS)(MV)(NL)(OJ)(PR)
WD1545+303 See also (NC)
WD1545+495 See also (NC)
WD1546+316 See also (NC)
WD1546+376 See also (QJ)(NC)
WD1546+426 See also (MS)
WD1547+015 See also (PP)
WD1547+390 See also (QJ)(NC)
WD1547+411 WD/MS eclipsing binary system. Ref.(PH) See also (QJ)(NC)(QH)(QN)
WD1548+405 See also (OK)
WD1548+539 See also (QJ)(NC)
WD1549-000 Correct Declination is +00 04 16 (1950). (DY)
WD1550+130 WD/MS eclipsing binary system. Ref.(PH)(QH)
WD1550+183 See also (PP)
WD1550+437 See also (NC)
WD1551+051 See also (NC)
WD1552+248 See also (QJ)
WD1552+486 See also (MS)
WD1553+414 See also (QJ)(NC)
WD1554+322 See also (OK)
WD1554+550 See also (NC)
WD1555+366 See also (NC)
WD1555+401 See also (NC)
WD1555-089 See also (PQ)
WD1556+026 See also (NC)
WD1556+085 See also (QJ)
WD1556+268 PCEB. Ref.(QH).
WD1558+378 Reclassified as M star; Ref.(QB)See also (NC)
WD1558+616 Name(s) for MS companion(s). HS 1558+6140B
WD1559+343 See also (NC)
WD1559+365 Irradiated secondary star; Cataclysmic variable? Ref.(QB)See also (QJ)(NC)
WD1559+366 See also (NC)
WD1559+369 R808 is a ZZ CETI variable, Ref.(7M) See also (PB)(NL) Polarized magnetic WD. Ref.(RG).
WD1559+534 See also (OK)
WD1600+308 See also (OK)
WD1600+472 DA; binary nature questionable.Ref.(QB)See also (NC)
WD1601+581 See also (QP)
WD1602+543 See also (NC)
WD1603+432 See also (QP)
WD1603+492 See also (PD)(MV)
WD1604+463 See also (QJ)(NC)
WD1605+089 See also (QJ)
WD1605+424 See also (QJ)(NC)
WD1605+428 See also (QJ)(NC)
WD1606+422 Double degenerate system. Ref.(JP) See also (NB)
WD1608+002 See also (QJ)(NC)
WD1608+258 See also (NC)
WD1609+011 See also (QJ)(NC)
WD1609+044 See also (PP)
WD1609+135 See also (PP)(OJ)(MY)
WD1609+468 See also (QJ)(NC)
WD1609+493 See also (QJ)(NC)
WD1611+459 See also (NC)
WD1611-084 See also (QM)
WD1613+458 See also (OW)
WD1614+136 See also (RL)
WD1614+160 See also (QV)
WD1615+390 See also (NC)
WD1615-154 See also (PP)(NB)(NL)(OK)
WD1616+010 See also (QJ)(NC)
WD1616+430 See also (NC)
WD1616+435 ZZ Ceti star Ref.(KB)
WD1617+064 Wide-binary? Ref.(QB)
WD1618-507.1 (P.Bergeron Finding Chart)
WD1619+123 Companion to HD 147528 Ref.(LJ)
WD1619+414 Name(s) for MS companion(s). KUV 16195+4125B
WD1619+525 Tertiary companion may be dM2; physical association of the three stars uncertain. Ref.(QO). See also (QR)(QP)
WD1620-391 CD-38 10980 25,000k DA degenerate with gravitational redshift, Ref.(CB)(JV), Companion to HD 147513.(LJ) See also (PP)(OS)(MV)(NL)(OK)(OJ)(PR)
WD1621+347 See also (QJ)(NC)
WD1621+360 See also (NC)
WD1621-002 See also (QJ)(NC)
WD1621-010 See also (NC)
WD1622+141 Reclassified as M star + nearby bright star; Ref.(QB)
WD1622+323 Name(s) for MS companion(s). PG 1622+323B See also (QP)
WD1622+369 See also (QJ)(NC)
WD1622+406 See also (NC)
WD1623+366 Probable double-degenerate system. Ref.(QT).
WD1623-540 See also (PR) (P.Bergeron Finding Chart)
WD1624+235 See also (QJ)
WD1625+125 ZZ Ceti (OC)
WD1626+291 See also (NC)
WD1626+368 See also (PS)(OJ)(NB)
WD1627+129 See also (QJ)
WD1626+495 See also (RF)(RS)
WD1628+390 See also (OK)
WD1628-873 (P.Bergeron Finding Chart)
WD1631+781 DA + DM detached binary RE1629+780, Ref.(AJ)(JV). Resolved triple (WD+dM3+dM3) system. Ref.(MQ) See also (QP)(QO)(QM)(NL)(RK)(SM)(SM)
WD1632+177 See also (QA)(OJ)
WD1632+387 DA; binary nature questionable.Ref.(QB)See also (NC)
WD1633+313 See also (NC)
WD1633+433 Member of binary or multiple star system. Ref.(OJ) See also (OH)
WD1633+572 CPM companion of CM Dra, Ref.(JV) See also (OJ)(PR)
WD1634-573 Hot (55,000K) DO degenerate with photospheric carbon in UV; hottest white dwarf with Einstein redshift, Ref.(AH)(AS)(JV).
WD1635+252 See also (NC)
WD1635+315 See also (NC)
WD1635+478 See also (NC)
WD1636+057 See also (PP)
WD1636+351 See also (QP)(JV)(NL)
WD1637+335 See also (NB)
WD1639+153 See also (MY)
WD1639+211 See also (NC)
WD1639+537 Only single magnetic degenerate with emission lines, Ref.(2H) See also (MV)
WD1640+113 See also (PP)
WD1640+384 See also (NC)
WD1641+114 See also (PP)
WD1641+241 See also (PD)(MV)
WD1641+387 See also (JV)
WD1643+143 Name(s) for MS companion(s). PG 1643+143B See also (QP)
WD1643+425 See also (NC)
WD1644+234 See also (QJ)
WD1644+424 PCEB (QH) See also (QJ)(NC)
WD1645+251 See also (NC)
WD1645+325 The first known pulsating DB white dwarf, Ref.(DW) See also (QP)(NB)
WD1645+372 See also (PD)(MV)
WD1646+062 Name(s) for MS companion(s). PG 1646+062B
WD1646+282 PCEB. Ref.(QH).
WD1646+361 See also (NC)
WD1647+591 G226-029 is a ZZ CETI variable, Ref.(7J); 1400A absorption, Ref.(3N) See also (PB)(PO)(MY)(NB)(NL)(OE)(OJ)
WD1648+342 See also (PD)(MV)
WD1648+371 See also (RY)
WD1648+391 See also (QJ)(NC)
WD1648+407 See also (JV)(NO)
WD1649+300 See also (NC)
WD1649+419 See also (NC)
WD1650+355 See also (PD)(MV)
WD1653+188 See also (NC)
WD1653+200 See also (NC)
WD1653+256 ZZ Ceti Candidate (Ref. JL)
WD1653+385 See also (PV)(OJ)
WD1654+160 V824 HER is a non-radial pulsator, Ref.(44), see section A5.23 in Ref.(LJ).
WD1655+215 See also (PP)(OJ)(NB)
WD1656-062 See also (PR)
WD1657+321 See also (OJ)
WD1657+343 See also (RK)(OK)(JV)
WD1658+440 Ultra-massive DA degenerate 1.31 MSUN, low B-field, X-ray source, Ref.(9U) See also (QP)(OQ)(8L)(5V)(JV)(MV)(RL)(RK)
WD1659+303 Finding chart for PG 1659+303B see A5.24 in Ref.(LJ)
WD1659+344 See also (NC)
WD1659+359 ZZ Ceti star Ref.(KB)
WD1659+442 See also (JV)
WD1659-531 BPM24601 common proper motion binary with HR6314 (F7 dwarf). Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart. See also (NB)(PR)
WD1701+596 See also (RF)(RS)
WD1702+322 See also (PD)(MV)
WD1703+199 See also (QJ)(NC)
WD1703+212 PCEB. Ref.(QH) See also (QJ)(NC)
WD1703+261 See also (PR)
WD1703+338 DA; binary nature questionable.Ref.(QB)
WD1703+388 See also (QJ)(NC)
WD1704+217 See also (NC)
WD1704+481.1 Sanduleak-Pesch binary pair of DA stars,12,500K, 9500K masses 0.08 and 0.43 solar masses,first known triple degenerate,average radial velocity=0.6km/sec, Ref.(9Q)(2E)(FH).
WD1704+481.2 Sanduleak-Pesch binary pair of DA stars,12,500K, 9500K masses 0.08 and 0.43 solar masses,first known triple degenerate,average radial velocity=0.6km/sec, Ref.(9Q)(2E)(FH).
WD1705+030 See also (PV)(OJ)
WD1706+220 See also (NC)
WD1706+332 See also (PQ)
WD1707+295 See also (NC)
WD1707+427 PG1159 DO degenerate, Ref.(DN); type A, Ref.(66) variable WD Ref(KL) Non-radial g-mode pulsator Ref.(KO)N.
WD1708+437 See also (QX)
WD1709+230 See also (OR)
WD1709-575 (P.Bergeron Finding Chart)
WD1710+559 See also (NC)
WD1710+683 Binary (DA7.2+K7/M0 dwarf) system. Ref.(MK) See also (PQ)(PR)
WD1711+305 MS+MS superposition; Ref.(QB)
WD1711+657 ZZ Ceti star Ref.(KB)
WD1711+668 See also (QM)
WD1712+274 See also (NC)
WD1712+298 See also (NC)
WD1712+629 See also (QJ)(NC)
WD1713+332 Double degenerate close binary, Ref.(7G).
WD1713+393 See also (MV)
WD1713+695 See also (QP)
WD1714-547 ZZ Ceti star ref.(KA) (P.Bergeron Finding Chart)
WD1715+547 See also (NC)
WD1715+601 See also (PD)(MV)
WD1716+020 Common proper motion binary. Ref.(JP) See also (PP)(NB)(PR)
WD1716+598 See also (NC)
WD1717+610 PCEB. Ref.(QH) See also (QJ)(NC)
WD1717-345 Possible red dwarf companion, Ref.(8P) See also (QO)
WD1719+560 See also (QJ)
WD1719+562 See also (PD)
WD1719+569 See also (QJ)(NC)
WD1719+629 See also (NC)
WD1720+283 See also (NC)
WD1720+638 See also (NC)
WD1722+541 See also (PD)(MV)
WD1723+553 Post-common envelope binary; irradiated secondary star. Ref.(QB)
WD1723+563 PCEB Ref.(QH) See also (QJ)(QH)(NC)
WD1723+586 ZZ Ceti star Ref.(KB) See also (NQ)(NL)
WD1723+595 See also (NC)
WD1724+626 See also (QJ)(NC)
WD1724-359 See also (RK)
WD1725+561 See also (QJ)(NC)
WD1725+586 See also (QM)(NO)(OK)(RK)
WD1726+545 Post-common envelope binary. Ref.(QB)See also (QJ)(NC)
WD1726-578 (P.Bergeron Finding Chart)
WD1727+589 See also (NC)
WD1728+565 See also (PD)(MV)
WD1728+621 See also (QJ)(NC)
WD1729+371 Contains circumstellar dust (NG) See also (QD)(QA)(OJ)(MR)
WD1730+625 PCEB. Ref.(QH) See also (QJ)(NC)
WD1731+591 ZZ Ceti star Ref.(KB)
WD1732+608 See also (NC)
WD1733-544 (P.Bergeron Finding Chart)
WD1734+542 See also (NC)
WD1734+742 Cataclysmic Variable of the RS CVn-type. Ref.(SM)
WD1735-318 An extremely hot DA white dwarf close to the open cluster NGC6405, Ref.(4P).
WD1736+052 See also (PP)
WD1736+133 White dwarf companion to HD160365, Ref.(36).
WD1736+540 See also (NC)
WD1736+562 See also (NC)
WD1738+669 Hottest known DA star associated with nebula, Ref.(12).
WD1740+541 See also (NC)
WD1740-706 See also (QM)(RL)
WD1741+543 See also (NC)
WD1743-521 (P.Bergeron Finding Chart)
WD1748+708 G240-072 is magnetic and polarized, Ref.(03) See also (MV)(NB)(NN)(OJ)
WD1750+098 EG124 common proper motion binary with G140-b1a / BD+09 3501 (K2 dwarf) See also (PQ).
WD1751+106 ABELL 43 is a hybrid, PG1159-like central star; type LGEH, Ref.(66) CSPN effective temperature 116,900K. (IO)N.
WD1756+143 See also (OJ)
WD1756+827 See also (OJ)(MM)(NB)(NN)(OL)
WD1800+685 See also (QP)(NL)(RK)
WD1802+213 See also (JV)
WD1803-482 RS CVn variable. Ref.(SM)
WD1814+248 A new magnetic degenerate, Ref.(8M).
WD1815+381 Variable polarized magnetic WD. Ref.(RG).
WD1818+126 See also (MV)
WD1819+580 See also (QM)(RK)
WD1820+609 See also (OJ)
WD1821+643 PG1159 DO degenerate, type LGE, Ref.(66)(JV)(KL) Non-radial g-mode pulsator Ref.(KO) See also (RN)
WD1822+008 SH2-68 is a PG1159-type planetary nucleus, type AH, Ref.(66) CSPN effective temperature 125,900K. (IO)N.
WD1822+410 See also (QA)(OB)
WD1823+063 NGC6633:LA15 = NGC6633:LAWDS15 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009
WD1824+040 Double-degenerate candidate Ref.(KP), Triple degenerate system DA3.4(a)+DC5.0(b)+DC10.6(c) see A5.1 in Ref.(LJ) Finding chart for G21-15C See also (PP)
WD1824+062 NGC6633:LA 8 = NGC6633:LAWDS 8 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009
WD1824+063 Calculated Mv=11.84 from model spectrum and radius and conclude star is too bright to be a member of NGC6633. (ED) nOTE: NGC6633:LA14 = NGC6633:LAWDS14
WD1824+063.1 NGC6633:LA27 = NGC6633:LAWDS27 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009
WD1824+063.2 NGC6633:LA13 = NGC6633:LAWDS13
WD1824+064 Possible double degenerate star, Ref.(MZ) Note NGC6633:LA 4 = NGC6633:LAWDS 4
WD1824+600 ZZ Ceti (OC)
WD1825+063 Possible double degenerate star, Ref.(MZ) Note NGC6633:LA 7 = NGC6633:LAWDS 7
WD1825+067 NGC6633:LA16 = NGC6633:LAWDS16
WD1826+064 NGC6633:LA12 = NGC6633:LAWDS12
WD1826-045 See also (QV)(OH)
WD1827-106 Temperatures ambigious. Ref.(PP) See also (OD)
WD1829+547 G227-035 is a magnetic white dwarf, Ref.(03) See also (OJ).
WD1830+721 HS1830-721 is an intermediate temperature DO star with TEFF > 80,000K, Ref.(2T).
WD1831-002 White dwarf companion of a binary pulsar, Ref.(9S).
WD1833+644 Possible triple-star system: DA2.0 with dM3+dM6.5 companions. Ref.(QO). See also (QP)
WD1834-781 (P.Bergeron Finding Chart) See also (PP)
WD1837-619 Strong UV lines of neutral carbon, Ref.(CI).
WD1840+042 See also (MY)
WD1844-223 See also (PP)(RK)
WD1844-654 See also (JV)
WD1845+019 Single-lined double-degenerate binary. Ref.(PP)See also (NL)(RK)
WD1845+683 White dwarf is likely, neither a suspected nor confirmed binary. Ref. (MQ) See also (PS)(NL)(NO)(RK)
WD1855+096 White dwarf companion of a binary pulsar, Ref.(9S).
WD1855+338 G207-009 is a ZZ CETI variable, Ref.(8Z) See also (PB)(MY)(NL)
WD1856+534 A possible triple system, Ref.(7Z).
WD1857+119 See also (PP)
WD1858+393 See also (QA)(MR)(OH)
WD1900+140 Central star of SH2-28; type A, Ref.(66).
WD1900+705 G260-015 is a magnetic white dwarf, Ref.(06)(03). See also (NB)(OJ)
WD1906-600 See also (JV)
WD1909+304 PG1159-like central star of NGC6765; type lgE, Ref.(66).
WD1910+047 Photospheric X-ray emission detected by HEAO-B, TEFF= 22,500K, Ref.(7D)(7B)(JV).
WD1911+135 See also (PP)(PQ)
WD1914+094 See also (PP)
WD1917+386 See also (OJ)
WD1917-077 LDS678A shows strong CI lines in UV, weak HeI in optical, Ref.(CF)(AO), Binary DA+dm3.5, Ref.(LJ) See also (PV)(OJ)(PR).
WD1918+376 See also (OS)
WD1919+145 See also (OJ)(NB)(NL)
WD1919+37602 Possible non-cluster WD. Ref.(NX)
WD1919+37603 Possible non-cluster WD. Ref.(NX)
WD1919+37605 Possible non-cluster WD; possible DA+dM binary system. Ref.(NX)
WD1919+37608 See also (OS)
WD1919+37610 Possible DA+dM binary system. Ref.(NX)
WD1921-566 See also (RK)
WD1929+011 See also (QV)
WD1930+278 See also (QX)
WD1932-136 See also (PP)(PR)
WD1935+276 G185-032 is a ZZ CETI variable, Ref.(7J) See also (PB)(NL)(OD)(OJ)
WD1936+327 See also (MZ)(NL)
WD1940+374 See also (OE)
WD1942+499 See also (NB)(NO)(RK)
WD1943+163 See also (PP)
WD1944-421 See also (JV)(SM)
WD1950+250 GR394 is a ZZ CETI variable, Ref.(86). See also (PB)
WD1950-432 See also (PP)(NO)
WD1953-011 See also (PP)(OJ)(MM)(NB)(NL)(OL)
WD1953-715 (P.Bergeron Finding Chart)
WD1957+225 Central star of PN. Ref.(QM) See also (QP)
WD1958+015 K1-18 is a PG1159-like central star of NGC6852, type lgE, Ref.(66).
WD1959+059 See also (PP)
WD2002-110 See also (OJ)(NN)
WD2003+437 GD387 probable unresolved DA+DC system, Ref.(23).
WD2003+542.1 See also (QX)
WD2004-605 See also (QM)(PP)(RK)
WD2007-219 See also (PP)
WD2007-303 See also (QP)(PP)(OJ)(NB)
WD2009+622 Name(s) for MS companion(s). GD 543B See also (QP)
WD2010+310 GD229 is magnetic and polarized, Ref.(6)(03); UV spectrum discussed in Ref.(1Q).
WD2011+398 PCEB DAQZ + dM3 binary. Ref.(RV)(10) See also(JV)(QO)(QM)(QH)(RK)
WD2014-575 See also (JV)(NB)(NL)(NO)
WD2019+756 MS+MS superposition; Ref.(QB)
WD2020-425 Double-lined double-degenerate binary. Ref.(PP)See also (JV)(NO)(RK)
WD2027+068 A new hot DO star with ultra highly excited ionization stages, Ref.(64).
WD2028+390 See also (JV)
WD2029+183 The finding charts point to different stars.
WD2031-277 See also (JV)
WD2032+188 Single-lined double-degenerate binary. Ref.(PP) See also (QX)
WD2032+248 See also (PV)(OJ)(JV)(NB)(NL)(OE)(RX)
WD2038-013 See also (NC)
WD2039-001 See also (MS)
WD2039-003 Reclassified as M star; Ref.(QB)See also (NC)
WD2039-202 See also (PP)(OJ)(NL)
WD2039-682 See also (PP)(OJ)(MV)(MY)(NB)
WD2040-392 See also (OJ)
WD2041-064 See also (NC)
WD2043-053 See also (QJ)(NC)
WD2043-073 See also (PD)(MV)
WD2043-635 See also (NO)
WD2044+001 See also (NC)
WD2044-043 See also (PQ)(PR)
WD2045+006 Low accretion rate polar. Ref.(QB)
WD2045-000 See also (NC)
WD2045-012 Reclassified as M star; Ref.(QB)
WD2046+396 See also (NL)
WD2046-059 See also (QJ)(NC)
WD2047+372 See also (OJ)(NB)(NL)
WD2047-000 Log g = 5; star is probably Main-sequence A-star. Ref.(QT).
WD2048+263 Member of binary or multiple star system. Ref.(OJ)
WD2048+809 See also (PQ)(PR)
WD2048-002 See also (QJ)(NC)
WD2048-250 See also (OJ)
WD2049-004 See also (PD)(MV)
WD2050-056 See also (RS)
WD2051+464 See also (JV)
WD2051-208 See also (PP)
WD2052+006 MS+MS superposition; Ref.(QB)See also (NC)
WD2053-011 DB; binary nature questionable.Ref.(QB)
WD2054+005 See also (QJ)(NC)
WD2054-050 See also (OJ)(NN)
WD2055+221 See section A1.1 in Ref. (LJ).
WD2056+033 See also (JV)
WD2056-062 See also (QJ)
WD2056-070 See also (NC)
WD2058+342.1 GD 392B is ultracool CPMB companion to GD 392 Ref.(JP)
WD2059+190 See also (MY)
WD2059+316 Strong UV CI lines, Ref.(CK).
WD2102+101 See also (NC)
WD2103-061 See also (QJ)(NC)
WD2104-070 See also (QJ)(NC)
WD2105-820 See also (QV)(QA)(PP)(OJ)(MV)(NB)(NL) (P.Bergeron Finding Chart)
WD2108+094 See also (QJ)(NC)
WD2109+010 See also (QJ)(NC)
WD2109+089 See also (RF)(RS)
WD2109+100 See also (QJ)(NC)
WD2110+102 DB; binary nature questionable.Ref.(QB)
WD2110-006 MS+MS superposition; Ref.(QB)
WD2111+498 See also (JV)(NB)(NL)(RX)(RK)
WD2111-012 PCEB Ref.(QH) See also (QJ)(NC)
WD2113+007 MS+MS superposition; Ref.(QB)
WD2114+239 The DAO degenerate central star of ABELL 74, Ref.(66).
WD2115+008 See also (QJ)(NC)
WD2115+118 A new hot DAO star with ultra highly excited ionization stages, Ref.(64).
WD2115+339 RXJ2117.1+3417 is a PG1159 star with 24 detected periods and an associated planetary nebula, Ref.(DF,BA); type lgE, Ref.(66)(JV) Non-radial g-mode pulstaor Ref.(KO)N.
WD2115-082 See also (NC)
WD2115-560 Contains circumstellar dust (NG) See also (QD)(QA)(PP)(OR)(OJ)(MV)(NB)
WD2116+736 See also (QP)(NO)(RK)
WD2116-005 Double-degenerate merger system. Ref.(QT).
WD2117+539 1400A absorption feature, Ref.(CL) See also (PV)(NL)(OJ)
WD2118-011 PCEB. Ref.(QH) See also (QJ)(NC)
WD2118-061 See also (NC)
WD2120+002 PCEB. Ref.(QH) See also (QJ)(NC)
WD2120+054 See also (PP)
WD2122+361 NGC7063:LA 3 = NGC7063:LAWDS 3
WD2122+362 NGC7063:LA 4 = NGC7063:LAWDS 4
WD2122+362.1 NGC7063:LA 1 = NGC7063:LAWDS 1
WD2122+362.2 NGC7063:LA 2 = NGC7063:LAWDS 2
WD2122+363 NGC7063:LA 6 = NGC7063:LAWDS 6
WD2122-013 WD is in a binary system with orbital period = 6.9 hours. Ref.(RU).See also (NC)
WD2123-226 White dwarf companion to the barium star ZETA Cap with MWD=0.96Msun TEFF= 23,200K, Ref.(35).
WD2124+191 PCEB. Ref.(QH)(RK)
WD2124+550 See also (MY)
WD2124-224 See also (QM)(PP)(RK)
WD2126+734 1400A absorption feature, Ref.(2I), (3N), Binary system - companion probable WD, see section A5.7 in Ref.(LJ) See also (NL)(OJ)
WD2126-069 Reclassified as M star + nearby bright star; Ref.(QB)
WD2127+115 PG1159 star. Ref.(QB)
WD2128+469 Eclipsing Binary system classified as a Cataclysmic Variable. (JF)(PH). See also (QH)(SM)(SM)
WD2129+000 See also (PR)
WD2129+003 PCEB. Ref.(QH) See also (QJ)(NC)
WD2129-002 Reclassified as M star + nearby bright star; Ref.(QB)
WD2130-047 See also (OB)
WD2131+066 PG1159 DO degenerate, Ref.(DN); type A, Ref.(66) Binary system: PG1159+M2V (IJ)N(KL)N Non-radial g-mode Pulsator Ref.(KO)N.
WD2132+096 See also (MR)
WD2134+125 High gravity PG1159-like central star of NGC7094, type lgEH, Ref.(66) CSPN effective temperature 125,900K. (IO)N.
WD2134+218 See also (PP)(NB)
WD2136+229 See also (PP)
WD2136+828 See also (NL)
WD2137+102 See also (QJ)(NC)
WD2138-332 See Also (NY)(OJ) See also (PV)
WD2139+115 See also (PP)
WD2140+207 Weak C2 reported, Ref.(5D) See also (PO)(OL)(NB)(JN)(OJ)(RQ)
WD2142+004 See also (QJ)
WD2142-169 See also (OR)
WD2143+108 CPMB with WD 2143+108.1. Ref.(SK)
WD2143+108.1 CMPB with WD 2143+108. Ref.(SK)
WD2144+128 See also (NC)
WD2144-004 See also (PY)
WD2144-079 See also (QA)(PS)(OR)
WD2146+005 See also (PD)(MV)
WD2146+412 Reclassified as a helium strong sub-dwarf B star.(EG) The coolest known DBA white dwarf; TEFF= 12,500K, Ref.(62).
WD2146-077 See also (PD)(MV)
WD2147+280 G188-27 shows weak HeI; coolest DB? Ref.(CE).
WD2148-075 DA; binary nature questionable.Ref.(QB) See also (QM)
WD2148-291 Short period ZZ Ceti (OC)
WD2149+000 See also (QJ)(NC)
WD2149+002 See also (MV)
WD2149+021 See also (QP)(QA)(PP)(MR)(NB)(NL)
WD2149+126 See also (PD)(MV)
WD2150+021 See also (PP)
WD2150-008 Noisy spectrum; Ref.(QB)See also (NC)
WD2151+125 Nearby bright star, binary nature questionable.; Ref.(QB) See also (QM)
WD2151-015 Name(s) for MS companion(s). LTT 8747B See also (QP)(RO)
WD2151-307 See also (RK)
WD2152-310 ZZ Ceti candidate (HC)
WD2152-548 See also (PP)(RK)(RK)
WD2153-419 See also (PP)(JV)(RK)
WD2154+408 WD2154+408 is a PCEB binary (P=0.26772 day) consisting of a hot white dwarf primary and a cool late MS companion. (HF)
WD2154-437 See also (PR)
WD2154-512 See also (OJ)(JV)(PR)
WD2155-009 See also (NC)
WD2157-074 See also (QJ)(NC)
WD2157-079 See also (OW)
WD2159-414 See also (PP)
WD2159-754 See also (OJ)
WD2200+113 See also (NC)
WD2200-000 See also (QJ)(NC)
WD2200-136 Double-lined double-degenerate binary. Ref.(PP)
WD2201-005 See also (QJ)(NC)
WD2202-282 ZZ Ceti candidate (HC)
WD2203+005 See also (NC)
WD2204-005 See also (QJ)(NC)
WD2204-012 See also (NC)
WD2205-015 WD+MS Eclipsing Binary System. Ref.(QN).
WD2205-139 See also (PP)
WD2206+121 See also (NC)
WD2207+121 See also (RF)(RS)
WD2207-004 See also (QJ)(NC)
WD2207-303 See also (NL)(RK)
WD2209-147 Double-lined double-degenerate binary. Ref.(PP) See also (QX)(QX)
WD2211+372 See also (PS)(MQ)
WD2211-316 ZZ Ceti candidate (HC)
WD2211-392 See also (OJ)
WD2211-495 See also (MV)
WD2212+656 The DA degenerate central star of IW2, Ref.(7U).
WD2213+007 PCEB. Ref.(QH) See also (NC)
WD2213+125 See also (QJ)(NC)
WD2214+005 See also (QJ)(NC)
WD2215+368 See also (OJ)
WD2215+388 GD 401 is a DB degenerate with upper limit calcium and magnesium abundances, Ref.(49). See also (PS)(QA)
WD2215-002 See also (PD)(MV)
WD2216+158 Double-lined double-degenerate binary. Ref.(PP)
WD2216+484 GD402 probable unresolved DA+DC system, Ref.(23).
WD2216-000 See also (QJ)(NC)
WD2216-657 L119-34, DZ star with rare carbon, Ref.(DE). See also (QA)(OV)
WD2218+002 See also (QJ)(NC)
WD2218+706 The DA central star of DEHT5, Ref.(7U).
WD2220+124 See also (QJ)(NC)
WD2220+133 See also (PP)(MY)(OK)
WD2221-165 See also (QV)(MR)
WD2223+130 See also (NC)
WD2224-004 See also (NC)
WD2224-009 See also (QJ)
WD2224-344 See also (PR)
WD2225+118 See also (RF)(RS)
WD2226+139 See also (NC)
WD2226-007 See also (QJ)(NC)
WD2226-210 Hydrogen dominated CSPN Ref.(KL)(SM)
WD2226-754 Wide CPM pair with WD2226-755 Ref. (FF) See also (PV)
WD2226-755 Wide CPM pair with WD2226-754 Ref. (FF) See also (PV)
WD2227-010 See also (QJ)(NC)
WD2227-010.1 See also (NC)
WD2228+126 See also (QJ)(NC)
WD2229+235 See also (QV)(MR)
WD2230+125 See also (NC)
WD2230-125 See also (PP)(MR)
WD2231-005 See also (NC)
WD2232+009 See also (NC)
WD2233+142 See also (NC)
WD2234-095 See also (NC)
WD2235-305 ZZ Ceti candidate (HC)
WD2236+129 See also (RF)(RS)
WD2237+000 CPMB with WD2237+000.1 (OM)
WD2237+000.1 CPMB with WD2237+000 (OM)
WD2237+143 See also (QJ)(NC)
WD2237-365 This is NOT LHS 3841 = LP 984-76 = Lephm 1-4978 as reported elswhere as per J.Farhi private communication 9/29/09 Finding Chart)
WD2238-098 PCEB. Ref.(QH) See also (QJ)(NC)
WD2239+001 See also (NC)
WD2240+125.1 A visual double DA binary, Ref.(2T).
WD2240+125.2 A visual double DA binary, Ref.(2T). See also (PP)
WD2240+217 Post-common envelope binary. Ref.(QB)
WD2240-017 See also (PP)
WD2241+009 See also (NC)
WD2242-002 See also (NC)
WD2244+030 = PG2244+031 Star A is the WD. Finding Chart see A5.12 in Ref.(LJ)
WD2245+146 See also (PD)(MV)
WD2246+120 Reported by Handler,G. 2001,MNRAS,323,L43 to be a pulsating DB White Dwarf of type V777Her
WD2246+223 See also (OJ)(MY)(NB)(NL)
WD2246-001 See also (NC)
WD2246-105 See also (NC)
WD2247+583 See also (RK)
WD2248+293 See also (OJ)(NN)
WD2249-105 See section A5.10 in Ref. (LJ).
WD2250-093 See also (NC)
WD2251-070 See also (QA)(PC)(OJ)(NN)
WD2252-005 See also (NC)
WD2253+054 Very weak spectrum, common proper motion pair. NOTE:Arizona Finding Chart points to 225553 +054530 See also(PR)
WD2253-081 G156-64 common proper motion binary with BD-8 5980 (G6 dwarf) See also (NZ)(PQ)
WD2254+126 ZZ Ceti star ref.(KA) See also (PP)
WD2256+249 GD245 is a composite DA + dM pre-cataclysmic binary, Ref.(9V) See also (MY)(OH)
WD2256+313 See also (PR)
WD2257+162 Name(s) for MS companion(s). PG 2257+162B
WD2257-073 DA + G5V binary, REF.(14).
WD2258+134 See also (QJ)(NC)
WD2258+155 See also (QC)
WD2258+406 See also (PQ)
WD2259+143 Hot/cold Table 1 temperatures ambigious. Ref.(PP)
WD2300-008 See also (QJ)(NC)
WD2301+762 See also (PR)
WD2301-072.1 CPM with WD2301-072.2, Ref.(3A).
WD2301-072.2 CPM with WD2301-072.1, Ref.(3A).
WD2303+242 KR Peg is a ZZ CETI variable, Ref.(44). See also (PB)
WD2303-005 See also (QJ)
WD2304+251 White dwarf companion to the mild barium star 56 PEG; may have accretion disk, Ref.(9T).
WD2306+124 See also (QC)(PP)
WD2308+050 See also (PP)
WD2309+006 See also (QJ)(NC)
WD2309+007 See also (QJ)(NC)
WD2309+105 See also (PP)(JV)(MZ)(NL)(RX)(RK)
WD2309-009 See also (RS)
WD2310+005 See also (NC)
WD2312-024 See also (QA)
WD2313-313 ZZ Ceti candidate (HC)
WD2315+003 See also (NC)
WD2315-098 PCEB. Ref.(QH) See also (QJ)(NC)
WD2316+123 New magnetic degenerate, with a 30Mg field, Ref.(5U).
WD2316-011 See also (NC)
WD2316-064 See also (PF)(MW)(NN)
WD2316-098 See also (QJ)(NC)
WD2316-173 IUE detection of CaII 1840A, Ref.(4L); strong UV CI lines, Ref.(CK).
WD2317+008 See also (PD)(MV)
WD2317+268 Name(s) for MS companion(s). KUV 23176+2650B
WD2317-295 ZZ Ceti candidate (HC)
WD2318+007.1 CPMB with WD 2318+007.2 Ref.(QL).
WD2318+007.2 CPMB with WD 2318+007.1 Ref.(QL).
WD2318+009 See also (NC)
WD2318+126 See also (PP)
WD2319+691.1 = A on Finding chart for GD 559B Ref.(LJ)
WD2319+691.2 = B on Finding chart for GD 559B Ref.(LJ)
WD2319-012 See also (QJ)(NC)
WD2320+003 See also (PD)(MV)
WD2321+005 See also (NC)
WD2321-010 See also (MV)
WD2321-549 See also (QM)(PP)(JV)(RK)
WD2322+118 See also (OR)
WD2322+137 See also (OJ)
WD2322-011.1 See also (NC)
WD2322-097 See also (QJ)(NC)
WD2322-181 See also (PP)
WD2323+157.2 Atmosphere virtually devoid of Hydrogen; Coolest known He atmosphere WD; Teff~3650K; Common proper motion pair with WD2323+157.1 (GD) Authors have witdrawn this paper. Star is a background subdwarf K7/M0 see A3.1 Ref.(LJ) see http://xxx.lan
WD2323-006 See also (NC)
WD2323-014 See also (NC)
WD2324+397 Peculiar PG1159-like degenerate star of type lgEH, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
WD2326+049 G029-038 is a ZZ CETI variable, Ref.(AE)(JE)(MR), Contains circumstellar dust (NG) See also (QV)(QD)(QA)(PP)(PB)(OR)(OH)(NL)(OJ)
WD2326-001 See also (NC)
WD2326-004 See also (NC)
WD2327+537 MS+MS superposition; Ref.(QB)
WD2328+107 See also (PP)
WD2329+134 See also (NC)
WD2329+267 See also (MV)
WD2329-090 See also (QJ)(NC)
WD2330-212 Single-lined double-degenerate binary. Ref.(PP)
WD2330-296 ZZ Ceti candidate (HC)
WD2331+290 Newly identified double degenerate close binary, Ref.(7G).
WD2331-005 See also (NC)
WD2331-475 See also (MV)(NB)(NL)
WD2333+301 WD associated with PN; Type: E Ref.(KL)
WD2333-007 See also (NC)
WD2333-049 See also (PS)(PP)
WD2334-139 See also (PP)
WD2335+305 JN1 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(DI); type E, Ref.(66).
WD2335-002 See also (NC)
WD2336-003 See also (QJ)
WD2336-005 See also (QJ)(NC)
WD2336-006 PCEB. Ref.(QH) See also (QJ)(NC)
WD2336-079 Long period ZZ Ceti (OC) See also (OJ)
WD2336-187 Double-lined double-degenerate binary. Ref.(PP)
WD2337-760 Double-degenerate candidate Ref.(KP).
WD2338+003 Post-common envelope binary. Ref.(QB) See also (QM)
WD2339+157 See also (QJ)(NC)
WD2339-100 See also (QJ)(NC)
WD2340+154 See also (QJ)
WD2341+322 EG162 common proper motion binary with G130-6 (M3 dwarf) See also (PV)(NL)(OJ)(PR)
WD2342+001 See also (QJ)
WD2342+806 GD561, the DAO central star of a newly discovered planetary nebula, Ref.(7T).
WD2343+386 See also (PD)(MV)
WD2343-005 Post-common envelope binary. Ref.(QB) See also (QM)
WD2343-008 See also (NC)
WD2343-106 See also (PD)(MV)
WD2343-176 See also (PP)
WD2344+434 See also (QJ)
WD2344-006 See also (QJ)(NC)
WD2344-266 See also (PR)
WD2345-089 See also (NC)
WD2345-313 ZZ Ceti candidate (HC)
WD2345-396 See also (PP)
WD2345-481 Single-lined double-degenerate binary. Ref.(PP)
WD2347+004 See also (QJ)
WD2347+128 ZZ Ceti star ref.(KA) See also (PP)
WD2347+292 See also (OJ)
WD2348-011 ZZ Ceti star Ref.(KB)
WD2348-244 EC23487-2424 is a ZZ CETI variable, Ref.(44). See also (PP)(PB)
WD2349+286 See also (NL)
WD2349-283 See also (PP)(MQ)
WD2349-364 See also (PP)
WD2350+001 See also (OY)
WD2350-083 The finding Charts place this star at 23 53 27.6 -8 4 41(2000) near the position of G273-B1A not G273-B1B. See also (PP)(PQ)
WD2350-248 See also (PP)
WD2350-279 ZZ Ceti candidate (HC)
WD2351+650.1 CPM WD component with M > 15.0, REF.(3A).
WD2351+650.2 CPM WD component with M > 15.0, REF.(3A).
WD2351-335 Triple system DA5.5+dM3.5+dM8 see A5.3 in Ref.(LJ) See also (OJ)(PQ)(PR)(RO)
WD2351-368 See also (PP)(MV)
WD2352+401 G171-027 has weak C2, Ref.(CE).
WD2354+159 See also (QA)(PS)(OR)
WD2354-151 See also (PP)
WD2357+296 See also (NL)
WD2359-324 See also (PP)
WD2359-434 See also (PP)(OJ)(NB)(OL)
WD1159-034 See also (SM)