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Interacting Magnetospheres in RS CVn Binaries – Coronal Heating and Flares
Published online by Cambridge University Press: 12 April 2016
Abstract
Coronae and flares of RS CVn systems are interpreted as due to gradual and sudden releases of magnetic free energy which is built up throught the interaction of magnetic fields of stars in these close binary systems.
- Type
- Session IV: Theoretical Aspects
- Information
- International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 629 - 632
- Copyright
- Copyright © Reidel 1983
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