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Theory of Magneto-Acoustic Modes in roAp Stars

Published online by Cambridge University Press:  12 April 2016

Lionel Bigot
Lionel Bigot*
Affiliation:
Niels Bohr Institute for Astronomy, Physics and Geophysics, Juliane Maries Vej 30, DK-2100 Copenhagen ∅, Denmark

Abstract

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In this review I present the effects of a strong magnetic field on the pulsations of rapidly oscillating Ap stars. I show how the field affects the observables, such as the frequencies and eigenvectors, and the selection of modes.

Type
Part 8. New theoretical developments in stellar pulsation and variability
Information
International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 445 - 452
Copyright
Copyright © Astronomical Society of the Pacific 2004

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