Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-15
Astronomy and Astrophysics
Astrophysics
3 pages, 1 figure, to appear in "Active OB Stars: Laboratories for Stellar & Circumstellar Physics", ASP Conf. Ser. 2005, S. S
Scientific paper
The stability of retrograde mixed modes in rotating B-type stars is
investigated. It is found that these modes are susceptible to kappa-mechanism
excitation, due to the iron opacity bump at log T ~ 5.3. The findings are
discussed in the context of the pulsation of SPB and Be stars.
No associations
LandOfFree
Kappa-Mechanism Excitation of Retrograde Mixed Modes in B-Type Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Kappa-Mechanism Excitation of Retrograde Mixed Modes in B-Type Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kappa-Mechanism Excitation of Retrograde Mixed Modes in B-Type Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-580347