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
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