FUSE Studies of Dwarf Novae During Quiescence

Details FUSE Studies of Dwarf Novae During Quiescence FUSE Studies of Dwarf Novae During Quiescence

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..194s&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Physics

Accretion, Acrretion Discs, Binaries: Close, Stars: Individual (Ww Ceti, Su Aur, Bv Cen, Ey Cyg)

Scientific paper

We have obtained FUSE spectra of several dwarf novae which reveal the properties of their accreting white dwarfs, their rates of accretion during quiescence and the nature of their boundary layer/inner disk regions including accretion belts on the white dwarfs. Among the systems for which preliminary results will be presented are BV Cen, WW Ceti, EY Cyg, SS Aur and VW Hyi. The contribution of these FUSE studies to our understanding of disk accretion physics will be emphasized within the context of the white dwarf and boundary layer.

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