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.
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Watson, M.G., King, A.R. & Heise, J. SS Cygni in outburst and quiescence. Space Sci Rev 40, 127–133 (1985). https://doi.org/10.1007/BF00212875
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DOI: https://doi.org/10.1007/BF00212875