Detection of X-ray emission from stellar coronae with ANS

Details Detection of X-ray emission from stellar coronae with ANS Detection of X-ray emission from stellar coronae with ANS

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202l..67m&link_type=abstract

Astrophysical Journal, vol. 202, Dec. 1, 1975, pt. 2, p. L67-L71.

Astronomy and Astrophysics

Astronomy

109

Astronomical Netherlands Satellite, Spaceborne Astronomy, Stellar Radiation, X Ray Astronomy, X Ray Stars, Binary Stars, Giant Stars, Main Sequence Stars, Stellar Mass Ejection, Supergiant Stars, Ultraviolet Radiation

Scientific paper

The soft X-ray detector aboard the Astronomical Netherlands Satellite (ANS) has been used to search for soft X-ray emission in the range 0.2 to 0.284 keV from hot stellar coronae. X-ray emission has been detected from Capella (alpha Aur) and Sirius (alpha CMa). For 26 other stars (main sequence, subgiants, giants, and supergiants) upper limits to the X-ray luminosity have been obtained. The physical conditions of a corona needed to explain the observations are discussed.

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