Ss-Cygni in Outburst and Quiescence

Details Ss-Cygni in Outburst and Quiescence Ss-Cygni in Outburst and Quiescence

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..127w&link_type=abstract

Space Science Reviews, Volume 40, Issue 1-2, pp. 127-133

Physics

17

Scientific paper

EXOSAT has been used to carry out a series of observations of the dwarf
nova SS Cygni covering both quiescent and outburst states which provide
a detailed picture of its behaviour at X-ray wavelengths. These results
provide strong support for a new coronal model for the X-ray emission
from non-magnetic white dwarf systems.

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