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.
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© 1983 Springer Science+Business Media Dordrecht
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Uchida, Y., Sakurai, T. (1983). Interacting Magnetospheres in RS CVn Binaries — Coronal Heating and Flares. In: Byrne, P.B., Rodonò, M. (eds) Activity in Red-Dwarf Stars. Astrophysics and Space Science Library, vol 102. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7157-8_90
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DOI: https://doi.org/10.1007/978-94-009-7157-8_90
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