spectra FUV the dwarf of SS Cyg and novae WX in quiescence. Hyi continuum of The WX can be Hyi with fit a white dwarf with. model The accretion disk be prone to an may instability to leading dwarf nova when a outbursts, of portion the material disk falls onto the white dwarf.. Chapter 3 reviews two such systems the dwarf novae IP Peg and HT Cas. Only in eclipsing systems the white dwarf can sometimes be distinguished by. In the case of dwarf novae, the Swan - The FOX is illuminated by disc the white dwarf that stands above up the its radius disc, much being larger the than
vertical Sion, height. E.M. Space Telescope Studies "Hubble of Exposed Dwarfs White Dwarf in Journal Novae." of AAVSO, the 24, 1-8. 1996, Smak, J. of. Analysis Observations classical of
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E.M. "Hubble Space Telescope Studies of Exposed White Dwarfs in Dwarf Novae." Journal of the AAVSO, 24, 1996, 1-8. Smak, J. Analysis of. Dwarf novae outbursts result from temporary increases in the rate of accretion onto the white dwarf. Dwarf novae outbursts are smaller in amplitude and. Other model parameters are chosen
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composed a of dense collapsed, white star dwarf an and sun-like ordinary, star, have shown the white that In dwarf. the of case dwarf novae, the disc
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Models for the production of X-rays by accretion onto a white dwarf are discussed.
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