VizieR

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

VizieR

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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. ((unassigned);meta.version;arith.diff;phys.veloc)
  (1)IRAS (char) IRAS name of object ((unassigned);meta.version;arith.diff;spect.line.veloc)
  (1+2+5)Name (char) Alternative identifications of object ((unassigned);pos.galactic.lon;arith.diff;spect.line.veloc;arith)
  (1+2)Teff K Effective temperature (Note 1)   ((unassigned);(unassigned);(unassigned);em.radio)
  (1)Dist pc (n) Distance (Note 2)   ((unassigned);(unassigned);(unassigned);em.UV.10-50nm)
  (1)b_Dist pc (n) 16th percentile of distance (Note 2)   ((unassigned);meta.version;arith.diff;em.UV.10-50nm)
  (1)B_Dist pc (n) 84th percentile of distance (Note 2)   ((unassigned);(unassigned);(unassigned);em.UV.10-50nm)
  (1+2)E(B-V) mag (n) Reddening ((unassigned);(unassigned);(unassigned);pos.lsr)
  (1+2)b_E(B-V) mag (n) Lower limit of reddening ((unassigned);(unassigned);(unassigned);phys.dust;arith.rate)
  (1+2)B_E(B-V) mag (n) Upper limit of reddening ((unassigned);meta.version;arith.diff;phys.dust;pos.lsr;meta.main)
  (1+2)Lum Lsun Luminosity (Note 3)   ((unassigned);(unassigned);(unassigned);(unassigned))

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2)b_Lum Lsun Lower limit of luminosity (Note 3)   ((unassigned);meta.version;arith.diff;(unassigned);arith.rate)
  (1+2)B_Lum Lsun Upper limit of luminosity (Note 3)   ((unassigned);(unassigned);(unassigned);(unassigned);pos.lsr;meta.main)
  (1+2)LIR % IR-to-stellar luminosity ratio ((unassigned);meta.version;arith.diff;(unassigned);instr.offset)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base ((unassigned);(unassigned);(unassigned);spect.line.veloc)
  (1+2+5)_RA deg Right Ascension (J2000) from SIMBAD (not part of the original data) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (1+2+5)_DE deg Declination (J2000) from SIMBAD (not part of the original data) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (2+5)Host (char) [SMC LMC] Host Magellanic Cloud ((unassigned);(unassigned);arith.factor;src.fwhm)
  (2)Ref (char) [a-d] Reference to the paper from which the object was taken (Note 1)   ((unassigned);meta.version;arith.diff;phys.size.diameter)
  (3+4)Mi Msun Initial mass ((unassigned);(unassigned);(unassigned);(unassigned))
  (3+4)MRLOF Msun Mass at the onset of RLOF ((unassigned);(unassigned);(unassigned);(unassigned))
  (3+4)logRRLOF [Rsun] Radius at the onset of RLOF ((unassigned);(unassigned);(unassigned);(unassigned))
  (3+4)qmin  Smallest mass ratio in the model grid for this primary model to result in stable mass transfer ((unassigned);(unassigned);(unassigned);(unassigned);src.orbital.inclination)
  (5)Porbmean d (n) Estimated orbital period determined from its luminosity (Note 1)   ((unassigned);(unassigned);(unassigned);phys.dust;meta.main)

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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Porbmin d (n) Estimated orbital period determined from the lower limit of its luminosity (Note 1)   ((unassigned);(unassigned);(unassigned);phys.dust;meta.main)
  (5)Porbmax d (n) Estimated orbital period determined from the upper limit of its luminosity (Note 1)   ((unassigned);(unassigned);(unassigned);phys.dust;meta.main)
  (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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Agemeansol yr Estimated post-mass-transfer age determined from its position in the HRD compared to the solar model grid ((unassigned);(unassigned);(unassigned);stat.filling;meta.main)
  (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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Ageminsol yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the solar model grid ((unassigned);(unassigned);(unassigned);stat.filling;arith.ratio)
  (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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Agemaxsol yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the solar model grid ((unassigned);(unassigned);(unassigned);stat.filling;pos.phaseAng;meta.main)
  (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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Agemeanmp yr Estimated post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid ((unassigned);(unassigned);(unassigned);stat.filling;meta.main)
  (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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Ageminmp yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid ((unassigned);(unassigned);(unassigned);stat.filling;arith.ratio)

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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Agemaxmp yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid ((unassigned);(unassigned);(unassigned);stat.filling;pos.phaseAng;meta.main)
  (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 ((unassigned);(unassigned);(unassigned);pos.eq.dec)

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