Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202l..73h&link_type=abstract
Astrophysical Journal, vol. 202, Dec. 1, 1975, pt. 2, p. L73-L76.
Astronomy and Astrophysics
Astronomy
80
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.
Brinkman Albert C.
den Boggende Antonius J. F.
Grindlay Jonathan
Gronenschild H. B. M. E.
Heise Jaret
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