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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
Abstract
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