The implications of disc instabilities on cataclysmic variable structure and evolution

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dc.creatorLasota, J. -P.
dc.date2004-02-09
dc.date.accessioned2026-07-07T02:12:11Z
dc.date.available2026-07-07T02:12:11Z
dc.descriptionApplications of the thermal-viscous disc instability model to various classes of cataclysmic variable very often require the accretion disc to be truncated. I argue that in most cases this inner truncation must be due to the white dwarf's magnetic field.
dc.descriptionTo appear in: Compact Binaries in the Galaxy and Beyond, IAU Coll. 194, editors E. Sion and G. Tovmassian
dc.identifierhttps://arxiv.org/abs/astro-ph/0402190
dc.identifierhttp://arxiv.org/abs/astro-ph/0402190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7368
dc.subjectAstrophysics
dc.titleThe implications of disc instabilities on cataclysmic variable structure and evolution
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