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Multi-Wavelength Observations of Stellar Flares

Published online by Cambridge University Press:  12 April 2016

P. B. Byrne
P. B. Byrne*
Affiliation:
Armagh Observatory, Armagh BT61 9DG, N. Ireland

Abstract

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We present observational data on stellar flares from a range of wavelength regimes, many of which were obtained simultaneously. Physical parameters of these flares are derived and discussed in the framework of the general solar flare model. It is found that flares on dMe stars are solar-like, except in mean energy. The parameters of flares on RS CVn stars are more extreme, however, and may require new models for their interpretation.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 104 , Issue 1: Solar and Stellar Flares , 1989 , pp. 61 - 74
Copyright
Copyright © Kluwer 1989

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