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Interacting Magnetospheres in RS CVn Binaries – Coronal Heating and Flares

Published online by Cambridge University Press:  12 April 2016

Y. Uchida  and
T. Sakurai
Y. Uchida
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, Japan
T. Sakurai
Affiliation:
Department of Astronomy, University of Tokyo, Japan

Abstract

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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

References

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