The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables

dc.creatorMauche, Christopher W.
dc.date1997-09-11
dc.date.accessioned2026-07-07T02:24:11Z
dc.date.available2026-07-07T02:24:11Z
dc.descriptionRecent 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 Discussed are EUV and X-ray light curves, dwarf nova oscillations, and spectra, with new and previously unpublished results on SS Cyg and OY Car.
dc.description8 pages, 4 Postscript figures; LaTeX format, uses paspconf.sty and epsf.sty; Submitted for inclusion in Proceedings of the 13th North American Workshop on Cataclysmic Variables, ed. S. Howell, E. Kuulkers, and C. Woodward (San Francisco: ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/9709101
dc.identifierhttp://arxiv.org/abs/astro-ph/9709101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11525
dc.subjectAstrophysics
dc.titleThe EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables
dc.typetext

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