Can the activity of the secondary components explain the X-ray emission from cataclysmic variables?

Details Can the activity of the secondary components explain the X-ray emission from cataclysmic variables? Can the activity of the secondary components explain the X-ray emission from cataclysmic variables?

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984obs...104..259r&link_type=abstract

The Observatory, vol. 104, p. 259-264 (1984)

Computer Science

2

Scientific paper

The accretion-powered emission of the primary components of cataclysmic binaries seems to dominate the observed X-ray fluxes; but in some dwarf-nova systems with relatively large secondary components this emission is close to, or only marginally exceeds, that expected from the secondary components on the assumption that for them LX/Lbol = 10-2, as is actually observed in rapidly rotating active M dwarfs.

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