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

  
J/A+A/466/277
  VLT-FLAMES survey of massive stars (Hunter+, 2007)
ReadMe+ftp
2007A&A...466..277H
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/466/277/stars(c)Star positions (49 rows)
2.J/A+A/466/277/abundEquivalent widths and abundances of the stars observed (tables 3, 4 and 5 of paper) (2793 rows)
3.J/A+A/466/277/table6Adopted atomic data for the absorption lines considered in this analysis (70 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)
   (1+2)VName (char) (i) Variable name (meta.id;meta.main)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)EW (char) Detailed abundances and equivalent widths for this star (meta.ref.url)
  (1)Obs (char) Display data from observations paper (meta.ref.url)
  (2+3)Species (char) Species of the element (phys.atmol.element)
  (2)n_Species (char) [B] B indicates a blend of lines (meta.note)
  (2+3)lambda 0.1nm Rest wavelength of the spectral line (em.wl;spect.line)
  (2)EW 0.1pm (n) Equivalent width (spect.line.eqWidth)
  (2)Abund [Sun] (n) Abundance of species, in [X/H] (phys.abund)
  (3)loggf [-] Oscillator strength value (phys.atmol.oscStrength)
  (3)Blends (char) Details of lines considered as blends (meta.ref;pos.frame)

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