X-rays from Cataclysmic Variables

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dc.creatorKuulkers, Erik
dc.creatorNorton, Andrew
dc.creatorSchwope, Axel
dc.creatorWarner, Brian
dc.date2003-02-18
dc.date2003-08-19
dc.date.accessioned2026-07-07T02:07:38Z
dc.date.available2026-07-07T02:07:38Z
dc.descriptionCataclysmic Variables are a distinct class of interacting binaries, transferring mass from a donor star to a degenerate accretor, a white dwarf. We here review X-ray observations of these systems, with some emphasis on what has been achieved in the last decade.
dc.description40 pages, 10 figures; minor updates to text. To appear in Compact Stellar X-Ray Sources, eds. W.H.G. Lewin and M. van der Klis, Cambridge University Press
dc.identifierhttps://arxiv.org/abs/astro-ph/0302351
dc.identifierhttp://arxiv.org/abs/astro-ph/0302351
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5759
dc.subjectAstrophysics
dc.titleX-rays from Cataclysmic Variables
dc.typetext

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