Periodicities in ASCA X-ray observations of Non-Magnetic Cataclysmic Variables

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dc.creatorBaskill, D. S.
dc.creatorWheatley, P. J.
dc.creatorOsborne, J. P.
dc.date2001-10-03
dc.date2001-11-06
dc.date.accessioned2026-07-07T02:00:37Z
dc.date.available2026-07-07T02:00:37Z
dc.descriptionWe have carried out a thorough analysis of non-magnetic cataclysmic variables observed with ASCA, and have discovered possible periods in three targets: WW Cet, EI UMa and IX Vel. These may be caused by the rotation of the white dwarf at the centre of the disk, or by the progression of a density wave in the inner accretion disk.
dc.description2 pages, uses newpasp.sty. To appear in `The Physics of Cataclysmic Variables and Related Objects', ASP Conf. Ser., eds. B.T. Gaensicke, K. Beuermann, K. Reinsch. Original poster available from http://www.star.le.ac.uk/~dbl/publications/
dc.identifierhttps://arxiv.org/abs/astro-ph/0110089
dc.identifierhttp://arxiv.org/abs/astro-ph/0110089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3468
dc.subjectAstrophysics
dc.titlePeriodicities in ASCA X-ray observations of Non-Magnetic Cataclysmic Variables
dc.typetext

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