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/journal_tables/A+A/276/389/

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J/A+A/276/389       The spectrum of FG Sge in 1992            (Kipper+, 1993)
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The spectrum of FG Sge in 1992
      Kipper T., Kipper M.
     <Astron. Astrophys. 276, 389 (1993)>
     =1993A&A...276..389K      (SIMBAD/NED BibCode)
================================================================================
Keywords: stars: chemically peculiar - abundances
ADC_Keywords: Abundances

Abstract:
   Wavelength measurements and line identifications from the 0.14A/pixel
   echelle spectra of FG Sge secured two weeks before the drastic dimming
   of the star in 1992 are presented. The abundances of 18 elements are
   derived. These abundances have not changed from 1986. The main features
   of the chemical composition of FG Sge atmosphere are the depletion of
   iron-group elements and the marked overabundances (up to 3 dex) of
   s-process elements. First time in the observational history of
   FG Sge C_2_ Swan bands are identified in its spectrum.

Objects:
    ----------------------------
       RA  (2000)  DE     Name
    ----------------------------
    20 11 55.8 +20 20 05  FG Sge
    ----------------------------

File Summary:
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  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table2             31     1545   Line identifications in FG Sge
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Byte-by-byte Description of file: table2
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   Bytes Format Units   Label     Explanations
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   1-  7  F7.2  0.1nm   LamObs    Measured wavelength
      14  I1    ---     Rc        Eye estimate of the residual intensity R_c_
                                   multiplied by 10
  17- 23  F7.2  0.1nm   Lam       []? Identification wavelength
  26- 30  A5    ---     Name      Name of the line identified
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(End)                                        Patricia Bauer [CDS]    1996-Jan-10
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