Observations of X-rays from flare stars with ANS

Details Observations of X-rays from flare stars with ANS Observations of X-rays from flare stars with ANS

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....1..154g&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 1. (A76-26851

Astronomy and Astrophysics

Astronomy

1

Astronomical Netherlands Satellite, Satellite Observation, Stellar Radiation, X Ray Astronomy, X Ray Sources, Background Radiation, Cosmic Rays, Light Emission, Radiant Flux Density, Radiation Detectors

Scientific paper

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

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