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J/A+A/434/1125
  B-type Supergiants in the SMC (Dufton+, 2005)
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2005A&A...434.1125D
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1.J/A+A/434/1125/table4Equivalent Widths Measurements and line-by-line abundances for SMC supergiants and AzV 304 (274 rows)

Simple ConstraintList Of Constraints
 
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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Name (char) Star name
  Spec (char) Ionic species of the element
  Lambda 0.1nm Rest wavelength of the spectral line
  n_Lambda (char) [B] B: the feature is a close doublet
  Exc eV Excitation of the lower level of the transition For close doublets the mean value is given
  loggf  Logarithm of the oscillator strength times degeneracy of the lower level. For doublets the value is the sum of the components
  EW pm Equivalent width of the star spectral lines
  Abund  Abundance estimate (Note 1)   

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