A STUDY OF THE ROLE OF Lyβ FLUORESCENCE ON O I LINE STRENGTHS IN Be STARS
The possibility of the Ly beta fluorescence mechanism being operational in classical Be (CBe) stars and thereby contributing to the strength of the O I [lambda]8446 line has been recognized for long. However, this supposition needs to be quantified by comparing observed and predicted O I line ratios...
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Veröffentlicht in: | The Astrophysical journal 2012-07, Vol.753 (1), p.1-8 |
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Sprache: | eng |
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