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The Temperatures of White Dwarfs in Accreting Binaries
DOI: 10.1007/3-540-51031-1_296
Bibcode: 1989LNP...328...92S
Szkody, Paula; Sion, Edward M.
Long-term observations of the dwarf nova WZ Sge with an outburst recurrence time of 33 years are studied. The results indicate that the UV flux reached an equilibrium value at about the end of 1986; this means that the UV flux continued to decrease for 8 years after outburst. If the underlying dwarf has provided a dominant amount of the UV flux si…
1989
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IAU Colloq. 114: White Dwarfs
IUE
6