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Asteroseismology of the Rapidly Oscillating Ap Stars

Published online by Cambridge University Press:  13 May 2016

L. Bigot
L. Bigot*
Affiliation:
Département CASSINI - Observatoire de la Côte d'Azur BP 4229-06304 - Nice cedex 4 - France

Abstract

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The pulsation properties of the rapidly oscillating Ap (roAp) stars are briefly presented. The combined effect of a strong magnetic field and rotation on pulsations is also discussed.

Type
Session I: Global Structure and Evolution of the Solar Interior
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 90 - 93
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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