VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
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J/A+A/703/A294
  Post-RGB binaries and stable mass transfer (Moltzer+, 2025)
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2025A&A...703A.294M
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/703/A294/tablec2(c)SED fitting results of the Galactic post-AGB and post-RGB binary sample (85 rows)
2.J/A+A/703/A294/tablec3(c)SED fitting results of the post-AGB and post-RGB binary candidate samples in the LMC and SMC (128 rows)
3.J/A+A/703/A294/tablec4Initial parameters of utilised stable mass transfer models with Z = 0.02 (111 rows)
4.J/A+A/703/A294/tablec5Initial parameters of utilised stable mass transfer models with Z = 0.00142 (118 rows)
5.J/A+A/703/A294/tablec7(c)Estimated orbital periods and post-mass-transfer ages of the post-RGB binary candidate subsamples in the LMC and SMC (75 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)IRAS (char) IRAS name of object (meta.id)
  (1+2+5)Name (char) Alternative identifications of object (meta.id;meta.main)
  (1+2)Teff K Effective temperature (Note 1)   (phys.temperature.effective)
  (1)Dist pc (n) Distance (Note 2)   (pos.distance)
  (1)b_Dist pc (n) 16th percentile of distance (Note 2)   (pos.distance)
  (1)B_Dist pc (n) 84th percentile of distance (Note 2)   (pos.distance)
  (1+2)E(B-V) mag (n) Reddening (phot.color.excess)
  (1+2)b_E(B-V) mag (n) Lower limit of reddening (phys.absorption;stat.min)
  (1+2)B_E(B-V) mag (n) Upper limit of reddening (phys.absorption;stat.max)
  (1+2)Lum Lsun Luminosity (Note 3)   (phys.luminosity)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2)b_Lum Lsun Lower limit of luminosity (Note 3)   (phys.luminosity;stat.min)
  (1+2)B_Lum Lsun Upper limit of luminosity (Note 3)   (phys.luminosity;stat.max)
  (1+2)LIR % IR-to-stellar luminosity ratio (phys.luminosity;arith.ratio)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (1+2+5)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (1+2+5)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (2+5)Host (char) [SMC LMC] Host Magellanic Cloud (meta.id.parent)
  (2)Ref (char) [a-d] Reference to the paper from which the object was taken (Note 1)   (meta.bib)
  (3+4)Mi Msun Initial mass (phys.mass)
  (3+4)MRLOF Msun Mass at the onset of RLOF (phys.mass)
  (3+4)logRRLOF [Rsun] Radius at the onset of RLOF (phys.size.radius)
  (3+4)qmin  Smallest mass ratio in the model grid for this primary model to result in stable mass transfer (phys.mass;meta.modelled)
  (5)Porbmean d (n) Estimated orbital period determined from its luminosity (Note 1)   (time.period)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)f_Porbmean   [0/1] If true (1), the orbital period is a lower limit as the luminosity of the object is larger than the maximum luminosity of the binary models (meta.code)
  (5)Porbmin d (n) Estimated orbital period determined from the lower limit of its luminosity (Note 1)   (time.period)
  (5)Porbmax d (n) Estimated orbital period determined from the upper limit of its luminosity (Note 1)   (time.period)
  (5)f_Porbmax   [0/1] If true (1), the maximum orbital period is a lower limit as the luminosity upper limit of the object is larger than the maximum luminosity of the binary models (meta.code)
  (5)Agemeansol yr Estimated post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age)
  (5)f_Agemeansol   [0/1] If true (1), the mean post-mass-transfer age is an upper limit, as the luminosity of the object is larger than the maximum luminosity of the solar model grid (meta.code)
  (5)Ageminsol yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age;stat.min)
  (5)f_Ageminsol   [0/1] If true (1), the minimum post-mass-transfer age is an upper limit, as the luminosity lower limit of the object is larger than the maximum luminosity of the solar model grid (meta.code)
  (5)Agemaxsol yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age;stat.max)
  (5)f_Agemaxsol   [0/1] If true (1), the maximum post-mass-transfer age is an upper limit, as the luminosity upper limit of the object is larger than the maximum luminosity of the solar model grid (meta.code)
  (5)Agemeanmp yr Estimated post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age)
  (5)f_Agemeanmp   [0/1] If true (1), the mean post-mass-transfer age is an upper limit, as the luminosity of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code)
  (5)Ageminmp yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age;stat.min)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)f_Ageminmp   [0/1] If true (1), the minimum post-mass-transfer age is an upper limit, as the luminosity lower limit of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code)
  (5)Agemaxmp yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age;stat.max)
  (5)f_Agemaxmp   [0/1] If true (1), the maximum post-mass-transfer age is an upper limit, as the luminosity upper limit of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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