Physics
Scientific paper
Mar 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361...45l&link_type=abstract
Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere
Physics
2
Scientific paper
A brief review of stellar pulsation in rotating stars is given, discussing the perturbation theory of rotation for slowly rotating stars, a numerical method used for rapidly rotating stars, and the traditional approximation for low frequency modes. As a formation mechanism of viscous decretion discs around Be stars, the wave-meanflow interaction formalism is applied to low frequency modes excited in SPB stars, to show that the surface rotation of the star is accelerated as a result of angular momentum redistribution by the oscillation modes.
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