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J/A+A/385/986       FUSE UV spectrum of HR 5223              (Fremat+, 2002)

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
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 1180Å). 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 (H2, 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
Byte-by-byte Description of file: table2.dat
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
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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