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Part of the book series: NATO ASI Series ((ASIC,volume 169))

Abstract

The discovery by Kurtz of phase coherent, rapid oscillations in certain Ap stars holds great promise for the new field of asterseismology. We discuss here a generalized oblique pulsator model for these stars which allows us to accurately compare the effects of rotation and magnetism. A central role for mode coupling and amplitude limitation in the observed period doubling is suggested.

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© 1986 D. Reidel Publishing Company, Dordrecht, Holland

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Dziembowski, W., Goode, P.R. (1986). Asterseismology for Certain Ap Stars. In: Gough, D.O. (eds) Seismology of the Sun and the Distant Stars. NATO ASI Series, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4608-8_46

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  • DOI: https://doi.org/10.1007/978-94-009-4608-8_46

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8547-2

  • Online ISBN: 978-94-009-4608-8

  • eBook Packages: Springer Book Archive

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