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Pulsation of Rotating and Magnetic Stars

Published online by Cambridge University Press:  12 April 2016

Sergei V. Vorontsov
Sergei V. Vorontsov*
Affiliation:
Institute of Astronomyand Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 OHA, EnglandandInstitute of Physics of the Earth, Moscow 123810, Russia(permanent address)

Abstract

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Rotation and a magnetic field break the spherical symmetry of a star viewed as a pulsating system, lifting the degeneracy of oscillation frequencies, and leading to (sometimes prominent) observational consequences. Theoretical studies of rotational and magnetic effects in pulsating stars are reviewed, starting with simple configurations with slow rotation and weak magnetic fields.

Type
VI. Asteroseismology: theory
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 497 - 511
Copyright
Copyright © Astronomical Society of the Pacific 1993

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