VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+A/703/A294
  Post-RGB binaries and stable mass transfer (Moltzer+, 2025)
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2025A&A...703A.294M
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Post annotation 		img(gal)
1.J/A+A/703/A294/tablec7Estimated 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: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
  Name (char) Identification (JHHMMSS.ss+DDMMSS.s or OGLE-LMC-T2CEP-NNN) ((unassigned);(unassigned);(unassigned);spect.line.veloc;arith)
  Host (char) [SMC LMC] Host Magellanic Cloud ((unassigned);phys.veloc.orbital;arith.diff;src.fwhm)
  Porbmean d (n) Estimated orbital period determined from its luminosity (Note 1)   ((unassigned);phys.veloc.orbital;arith.diff;phys.dust;meta.main)
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  Porbmin d (n) Estimated orbital period determined from the lower limit of its luminosity (Note 1)   ((unassigned);phys.veloc.orbital;arith.diff;phys.dust;meta.main)
  Porbmax d (n) Estimated orbital period determined from the upper limit of its luminosity (Note 1)   ((unassigned);phys.veloc.orbital;arith.diff;phys.dust;meta.main)
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  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)
  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 (phot.color;instr.det.noise;arith.grad;pos.eq.dec)
  Ageminsol yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the solar model grid ((unassigned);phys.veloc.orbital;arith.diff;stat.filling;arith.ratio)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  Agemaxsol yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (src.veloc.lsr;(unassigned);arith;stat.filling;pos.phaseAng;meta.main)
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  Agemeanmp yr Estimated post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid ((unassigned);phys.veloc.orbital;arith.diff;stat.filling;meta.main)
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  Ageminmp yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid ((unassigned);phys.veloc.orbital;arith.diff;stat.filling;arith.ratio)
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  Agemaxmp yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid ((unassigned);phys.veloc.orbital;arith.diff;stat.filling;pos.phaseAng;meta.main)
  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);phys.veloc.orbital;arith.diff;pos.eq.dec)
  _RA deg Positions from Name and Simbad (right ascension part) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned);arith)
  _DE deg Positions from Name and Simbad (declination part) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned);arith)

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