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Acoustic wave driven mass loss in late-type giant stars
Published online by Cambridge University Press: 04 August 2017
Abstract
Mass loss generated by radiatively damped acoustic waves is investigated. We find that a persistent wave energy flux leads to extended chromospheres. Mass loss is quite likely produced if the wave field retains a transient character and if large wave periods are used.
- Type
- Mass-Loss From Cool Stars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 325 - 326
- Copyright
- Copyright © Reidel 1987
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