Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

Details Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085 Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196...95s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 196, July 1981, p. 95-100. Research supported by the Science Research C

Astronomy and Astrophysics

Astronomy

33

Flare Stars, Stellar Luminosity, Stellar Radiation, X Ray Sources, Ariel 5 Satellite, Binary Stars, Light Curve, Stellar Coronas, X Ray Stars

Scientific paper

We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.

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