The The structure of the Si IV region in Be stars: a study of Si IV spectral lines in Be 68 stars

The The structure of the Si IV region in Be stars: a study of Si IV spectral lines in Be 68 stars

Using the GR model, we analyze the UV Si IV resonance lines in the spectra of 68 Be stars of different spectral subtypes, in order to detect the structure of Si IV region. We calculated the values of the rotational, radial and random velocities as well as the absorbed energy of each one of the λλ 13...

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Veröffentlicht in:Journal of physics. Conference series 2012-01, Vol.399 (1), p.12021-7
Hauptverfasser: Antoniou, A, Danezis, E, Lyratzi, E, Stathopoulos, D
Format: Artikel
Sprache:eng
Schlagworte:
B stars
Line spectra
Mathematical models
Physics
Resonance
Resonance lines
Rotational
Silicon
Spectral lines
Stars
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Zusammenfassung:Using the GR model, we analyze the UV Si IV resonance lines in the spectra of 68 Be stars of different spectral subtypes, in order to detect the structure of Si IV region. We calculated the values of the rotational, radial and random velocities as well as the absorbed energy of each one of the λλ 1393.755, 1402.778 Å Si IV resonance lines and we present the relation between some of these parameters and their variation as a function of the spectral subtype.
ISSN:1742-6588
1742-6596
DOI:10.1088/1742-6596/399/1/012021