Ss-Cygni in Outburst and Quiescence
DOI: 10.1007/BF00212875
Bibcode: 1985SSRv...40..127W
Heise, J.; King, A. R.; Watson, M. G.
United Kingdom, Netherlands
Abstract
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.
1985
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Space Science Reviews
Exosat
21