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On the Mechanism of Mode Selection in Rapidly-Oscillating Magnetic Ap-Stars

Published online by Cambridge University Press:  12 April 2016

I. W. Roxburgh  and
S. V. Vorontsov
I. W. Roxburgh
Affiliation:
Astronomy Unit, Queen Mary and Westfield College, Mile End Road, London El 4NS, UK
S. V. Vorontsov
Affiliation:
Astronomy Unit, Queen Mary and Westfield College, Mile End Road, London El 4NS, UK

Abstract

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We address the problem of the preferential mode excitation in magnetic Ap-stars by estimating the pulsation energy losses in the atmosphere through the generation of the Alfvenic waves.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 343 - 344
Copyright
Copyright © Astronomical Society of the Pacific 1995

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