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

  
J/A+A/434/1125
  B-type Supergiants in the SMC (Dufton+, 2005)
ReadMe+ftp
2005A&A...434.1125D
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/434/1125/table1(c)Observational summary of the nine program stars and AzV 304 (10 rows)
2.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
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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)Name (char) (i) Star name
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000.0), from Simbad (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000.0), from Simbad (pos.eq.dec;meta.main)
  (1)Vmag mag Visual V magnitude
  (1)SpType (char) MK spectral type
  (1)S/N  (n) Signal-to-noise ratio
  (1)HRV km/s (n) Heliocentric radial velocity
  (1)FWHM km/s (n) FWHM of the metal absorption line spectrum
  (2)Spec (char) Ionic species of the element
  (2)Lambda 0.1nm Rest wavelength of the spectral line
  (2)n_Lambda (char) [B] B: the feature is a close doublet
  (2)Exc eV Excitation of the lower level of the transition For close doublets the mean value is given
  (2)loggf  Logarithm of the oscillator strength times degeneracy of the lower level. For doublets the value is the sum of the components
  (2)EW pm Equivalent width of the star spectral lines
  (2)Abund  Abundance estimate (Note 1)   

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