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/journal_tables/A+A/385/986/

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J/A+A/385/986       FUSE UV spectrum of HR 5223              (Fremat+, 2002)
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FUSE observations towards the pole-on Be star HR 5223.
     Fremat Y., Zorec J., Hubert A.-M., Cidale L.S., Rohrmann R.D.,
     Desert J.-M., Ferlet R., Vidal-Madjar A.
    <Astron. Astrophys. 385, 986 (2002)>
    =2002A&A...385..986F
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ADC_Keywords: Stars, emission - Spectra, ultraviolet
Mission_Name: FUSE
Keywords: stars: emission-line, Be - stars: fundamental parameters -
          stars: individual: HR 5223 - stars: rotation - ISM: abundances -
          stars: distances

Abstract:
    New spectra have been obtained for the pole-on Be star HR 5223 (HD
    120991) using the Far Ultraviolet Satellite Explorer (FUSE). We give a
    complete description of the far-UV spectral range (920 to 1180{AA}).
    The spectra are affected by strong blends with interstellar lines and
    molecular bands that also significantly lower the energy distribution
    of the star. We produce a synthetic spectrum of the interstellar
    medium (ISM) to determine the column densities of several elements
    (H_2_, H I, N I, O I ...) seen towards HR 5223 and to disentangle the
    components due to the ISM, the photosphere and/or to the circumstellar
    envelope.

Objects:
    ----------------------------------------------------------
       RA   (2000)   DE      Designation(s)
    ----------------------------------------------------------
    13 53 57.2   -47 07 41   HR 5223 = HD 120991
    ----------------------------------------------------------

File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe          80        .   This file
table2.dat      24      460   Photospheric and interstellar line
                                 identification list
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  7  F7.2  0.1nm   Wobs      Observed wavelength
   9- 15  F7.2  0.1nm   Wth       Theoretical wavelength
  17- 23  A7    ---     Id        Line identification
      24  A1    ---   n_Id        [*] *: photospheric line
--------------------------------------------------------------------------------

History:
    From electronic version of the journal
================================================================================
(End)                                        Patricia Bauer [CDS]    26-Apr-2002
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