X-ray emission from non-magnetic cataclysmic variables

Details X-ray emission from non-magnetic cataclysmic variables X-ray emission from non-magnetic cataclysmic variables

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..225v&link_type=abstract

(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque

Astronomy and Astrophysics

Astrophysics

7

Cataclysmic Variables, Exosat Satellite, Stellar Activity, Stellar Coronas, X Ray Binaries, Accretion Disks, X Ray Spectra

Scientific paper

EXOSAT observations of a large sample of non-magnetic cataclysmic variables have led to the detection of VW Hyi and OY Car as strong soft X-ray sources during superoutburst. The spectral characteristics of the X-ray emission of these SU UMa systems are compared. It is proposed that both systems have, besides a cool, optically thick boundary layer, an extended hot, optically thin corona.

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