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Asteroseismology of rapidly rotating pulsators
Published online by Cambridge University Press: 21 October 2010
Abstract
Oscillation frequencies were determined for a number of rapidly rotating main sequence stars. However, real seismic probing is still ahead of us. I review here tools that we have for modeling pulsation in rotating stars and their potential application to seismic sounding.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 360 - 361
- Copyright
- Copyright © International Astronomical Union 2010
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