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Detailed Description of J/A+AS/131/479
J/A+AS/131/479      Spectroscopy of MWC 297 (Andrillat+ 1998)
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B[e] stars. VI. MWC 297 = IRAS 18250-0351
       Andrillat Y., Jaschek C.
      <Astron. Astrophys. Suppl. Ser. 131, 479 (1998)>
      =1998A&AS..131..479A      (SIMBAD/NED BibCode)
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ADC_Keywords: Equivalent widths ; Spectra, infrared ; Stars, emission
              Stars, early-type
Keywords: stars: MWC 297 = IRAS 18250-0351 - stars, Be - stars: peculiar -
          stars: variable

Abstract:
    On the basis of spectroscopic CCD material obtained at the Haute
    Provence Observatory, we provide line identifications and equivalent
    width measurements in the wavelength region 4100-8900Å of the
    spectrum of MWC 297. About two hundred features are identified, almost
    exclusively emission lines. Only one interstellar feature could be
    identified ({lambda}6613) a fact which contrasts with the eigth
    magnitudes of extinction found by photometrists. The spectrum of the
    underlying star corresponds probably to a late O or early B-type
    object. The cooler emission lines correspond to a spectrum of a middle
    A-type star. Analogies with other stars observed in this series of
    papers are examined.
Objects:
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       RA   (2000)   DE    Designation(s)
    ----------------------------------------------------------
    18 27 39.5 -03 49 52   MWC 297 = IRAS 18250-0351 = NZ Ser
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File Summary:

FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 80 194 Equivalent widths and line identifications in the spectra of MWC 297
See also: J/A+AS/117/281 : Spectroscopy of HD 51585 (= OY Gem) (Jaschek+, 1996) J/A+AS/118/495 : Spectroscopy of MWC 349 A (Andrillat+ 1996) J/A+AS/120/99 : Spectroscopy of MWC 645 (Jaschek+, 1996) J/A+AS/124/441 : Spectroscopy of HD 45677 = MWC 142 (Andrillat+ 1997) J/A+AS/128/475 : Spectroscopy of MWC 158 (Jaschek+ 1998) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 7 F7.2 0.1nm LambdaMea Measured wavelength 8- 9 A2 --- Line [ea&] Emission (e) or absorption (a) line 11- 17 F7.3 0.1nm EW ? Equivalent width 18- 20 A3 --- n_EW Note on EW (1) 22- 26 F5.2 0.1nm LambdaLab ? Laboratory wavelength 28- 32 F5.2 0.1nm DLambda ? Measured minus laboratory wavelength 34- 80 A47 --- Ident Line Identification and comments (2)
Note (1): +f: refers to the following line w: wide Note (2): bl: blend Prob: probability Coinc: coincident
History: Prepared via OCR at CDS. ================================================================================ (End) Patricia Bauer [CDS] 16-Jun-1998
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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