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Asteroseismology of rapidly rotating pulsators

Published online by Cambridge University Press:  21 October 2010

W.A. Dziembowski
W.A. Dziembowski*
Affiliation:
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland email: wd@astrouw.edu.pl Copernicus Astronomical Center, ul. Bartycka 18, 00-716 EarszawaPoland
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Abstract

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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.

Keywords

stars: oscillations - stars: rotation
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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