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  IRAS 20004+2955 (V1027 Cyg) chemical comp. (Klochkova+, 2000)
Post annotation
1.J/PAZh/26/465/table2Atomic data, equivalent widths of special lines and elemental abundances for two atmosphere models (115 rows)
2.J/PAZh/26/465/table3Atmospheric elemental abundances for V1027 Cyg (19 rows)

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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)
   (ALL)El (char) Element (phys.atmol.element)
  (1)Lambda 0.1nm Wavelength (em.wl)
  (1)ExcPot eV Excitation potentials of the lower level (;phys.atmol.excitation)
  (1)Loggf  Oscillator strength (log gf) (phys.atmol.wOscStrength)
  (1)EW 0.1um Equivalent width (spect.line.eqWidth)
  (1)A(X)1  Chemical composition for the model: Teff=5000K, logg=1.0 (phys.abund)
  (1)A(X)2  Chemical composition for the model: Teff=4900K, logg=0.5; (phys.abund)
  (2)n  Number of the lines used (meta.number)
  (2)logA1  Mean atmospheric elemental abundances for Teff=5000K, logg=1.0 (phys.abund)
  (2)e_logA1  (n) rms uncertainty on logA1 (stat.error)
  (2)logA2  Mean atmospheric elemental abundance for Teff=4900K, logg=0.5 (phys.abund)
  (2)e_logA2  (n) rms uncertainty on logA2 (stat.error)
  (2)logASun  Solar atmospheric elemental abundance (phys.abund)

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