VizieR

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VizieR

  
J/A+A/581/A22
  67 CEMP-s stars model analysis (Abate+, 2015)
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1.J/A+A/581/A22/table3Physical parameters of the model CEMP-s stars with nu>=2 computed with model set B with WRLOF wind-accretion efficiency and spherically symmetric wind (43 rows)

 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. ((unassigned);(unassigned);stat.min;phys.veloc)
  Sample (char) Sample (Note G1)   ((unassigned);(unassigned);(unassigned);pos.parallax.trig;meta.main)
  Name (char) Star name ((unassigned);meta.version;arith.diff;spect.line.veloc;arith)
  M1i Msun Primary mass fitted parameter, M1,i ((unassigned);meta.version;arith.diff;(unassigned))
  MPMZ d Mass of the PMZ fitted parameter, MPMZ ((unassigned);(unassigned);(unassigned);(unassigned))
  M2i Msun Secondary mass fitted parameter, M2,i ((unassigned);meta.version;arith.diff;(unassigned))
  Pi d Orbital period fitted parameter ((unassigned);meta.version;arith.diff;phys.dust;meta.main)
  DMacc Msun Mass accreted by the secondary star, {Delta}Macc ((unassigned);meta.version;arith.diff;(unassigned))
  Pf d Orbital period of the binary when the secondary star best reproduces the observed logg and surface abundances ((unassigned);meta.version;arith.diff;phys.dust;meta.main)
  PfI d (n) Final period determined in paper I (Abate et al., 2015A&A...576A.118A) (except in tables a4 and a7) ((unassigned);meta.version;arith.diff;phys.dust;meta.main)
  chi2min  Minimum chi2 ((unassigned);(unassigned);(unassigned);time.resolution;meta.main)
  nu  Number of degrees of freedom of the fit ((unassigned);meta.version;arith.diff;src.var)
  chi2/nu  (n) Reduced chi2R of the best fit ((unassigned);meta.version;arith.diff;phys.veloc.orbital)
  all  Display data for all models ((unassigned);meta.version;arith.diff;pos.geocentric)

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