Multi-wavelength observations of stellar flares

Details Multi-wavelength observations of stellar flares Multi-wavelength observations of stellar flares

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121...61b&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Astronomy and Astrophysics

Astronomy

33

Astronomical Models, Solar X-Rays, Stellar Flares, Iue, Mass Transfer, Stellar Models, Stellar Spectra, Ultraviolet Astronomy

Scientific paper

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.

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