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J/AJ/149/59
  Abundances of ρ Pup (Yushchenko+, 2015)
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2015AJ....149...59Y
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1.J/AJ/149/59/table2Abundances of chemical elements in the atmosphere of ρ Pup: individual lines (430 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. (meta.record)
  Tel (char) Telescope facility used (IUE or VLT) (Note G1)   (meta;instr.setup)
  M  Mean abundance for this element (meta.ref.url)
  Ion (char) Species identifier (phys.atmol.ionStage)
  lambda 0.1nm [1942/9797] Wavelength λ; in Å (em.wl)
  loggf [-] [-5.69/1.29] Log of the oscillator strength (phys.atmol.oscStrength)
  r_loggf  Reference for loggf (Note G2)   (meta.ref;phys.atmol)
  Elow eV [0/12.729] Lower level energy (phys.energy;phys.atmol.level)
  logN* [-] Log number absolute abundance in ρ Pup (Note G3)   (phys.abund)
  logNo [Sun] (n) Log number absolute abundance in the Sun (Note G3)   (phys.abund)
  Abund [Sun] Difference between logN* and logNS (Note 1)   (phys.abund;arith.diff)
  Inp*  Relative input of the investigated line to the line absorption coefficient in synthetic spectrum of ρ Pup (1=Clean line, 0=Very weak line) (Note 2)   (meta.note)
  Inpo  (n) Relative input of the investigated line to the line absorption coefficient in synthetic spectrum of the Sun (1=Clean line, 0=Very weak line) (Note 2)   (meta.note)
  Depth*  Depth of line in synthetic spectrum of ρ Pup (phys.absorption.opticalDepth)
  Deptho  (n) Depth of line in synthetic spectrum of the Sun (phys.absorption.opticalDepth)
  d(T) [-] (n) Change in logN* for Teff=+100K (Note 3)   (phys.abund)
  d(g) [-] (n) Change in logN* for logg=-0.3 (Note 3)   (phys.abund)

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