Linear, nonadiabatic pulsation calculations for models of upper main sequence and $\beta$ cephei stars
| Author | |
|---|---|
| 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
|
| Start Page or Article ID |
135-146
|
| Publisher |
"Springer Berlin Heidelberg"
|
| Conference Location |
"Berlin, Heidelberg"
|
| ISBN Number |
"978-3-540-39297-2"
|
| DOI |
10.1007/3-540-09994-8_12
|
| Download citation | |
| Publication Status | |
| JILA PI | |
Conference Proceedings
|