The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables

Details The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables

1997-09-11

arxiv.org/abs/astro-ph/9709101v1

Astronomy and Astrophysics

Astrophysics

8 pages, 4 Postscript figures; LaTeX format, uses paspconf.sty and epsf.sty; Submitted for inclusion in Proceedings of the 13t

Scientific paper

Recent results are presented and discussed regarding the EUV and X-ray emission of nonmagnetic cataclysmic variables. Emphasis is given to high accretion rate systems (novalike variables and dwarf novae in outburst), and to a number of apparent discrepancies between observations and the theory of the boundary layer between the accretion disk and the surface of the white dwarf. Discussed are EUV and X-ray light curves, dwarf nova oscillations, and spectra, with new and previously unpublished results on SS Cyg and OY Car.

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