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Multi-wavelength observations of stellar flares

✍ Scribed by P. B. Byrne

Publisher
Springer
Year
1989
Tongue
English
Weight
658 KB
Volume
121
Category
Article
ISSN
0038-0938

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✦ Synopsis

We present observational data onsteUar flares from a range of wavelength regimes, many of winch 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.

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✍ Robert A. Stern πŸ“‚ Article πŸ“… 1987 πŸ› Springer 🌐 English βš– 198 KB

It is now more than ten years since the first x-ray emitting stellar corona was discovered (Catura, Acton, and Johnson 1975). Since then, rapid progress has been made in cataloging the incidence and range of stellar x-ray emission, most notably with the Einstein Observatory (see, eg., reviews by Ste