Evidence for X-ray emission from flare stars observed by ANS

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Netherlands Satellite, Background Radiation, Galactic Radiation, Spaceborne Astronomy, Stellar Radiation, X Ray Astronomy, Astronomical Models, Flares, Light Emission

Scientific paper

Observations that detected the first X-ray emission from flare stars are described. An X-ray flare was detected from YZ CMi at 0.28 keV and approximately 1-7 keV, although no optical or radio coverage was available. During a very large optical flare from UV Ceti, X-ray emission at (only) 0.28 keV was detected. Upper limits for X-ray emission from several small optical flares of UV Ceti are presented. Implications for X-ray flare models, the diffuse X-ray background, and low-energy cosmic-ray flux are mentioned.

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