arXiv · astro-ph/9709101
The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables
Abstract
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 Discussed are EUV and X-ray light curves, dwarf nova oscillations, and spectra, with new and previously unpublished results on SS Cyg and OY Car.
Explore related subjects
Keep this discovery
Christopher W. Mauche. 1997-09-11. The EUV and X-ray Emission of Nonmagnetic Cataclysmic Variables. https://arxiv.org/abs/astro-ph/9709101
Cite the original work for its findings. Save a collection to share your selection of sources.