Linear, nonadiabatic pulsation calculations for models of upper main sequence and $\beta$ cephei stars
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Abstract |
Equations for linear nonadiabatic pulsation and the method of their solution are discussed in some detail. The numerical results presented concern mainly 7 M$\delta$ stellar models in early evolutionary phase. A driving zone at a temperature of 1.5 x 105 K was found to be present for both radial and nonradial modes, but no net pulsational instability was observed. Effects of rotation on pulsation frequencies and on stability are also discussed. |
Year of Conference |
2005
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Start Page or Article ID |
135-146
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Publisher |
"Springer Berlin Heidelberg"
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Conference Location |
"Berlin, Heidelberg"
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ISBN Number |
"978-3-540-39297-2"
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DOI |
10.1007/3-540-09994-8_12
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Publication Status | |
JILA PI | |
Conference Proceedings
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