The Turn-off of Classical Novae Observed Through X-rays: Models versus ROSAT Observations of V1974 Cyg

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dc.creatorSala, Gloria
dc.creatorHernanz, Margarita
dc.date2004-10-05
dc.date.accessioned2026-07-07T02:14:54Z
dc.date.available2026-07-07T02:14:54Z
dc.descriptionDetection of X-ray emission from classical novae in their post-outburst stages provides crucial information about the nova phenomenon. The soft X-ray emission gives a direct insight into the remaining hot nuclear burning shell. A numerical model for steady H-burning white dwarf envelopes has been developed to study the post-outburst phases of classical novae. Properties of the X-ray emission of the post-nova white dwarf are obtained, and the results are compared to ROSAT observations of V1974 Cyg.
dc.description2 pages. To appear in "The astrophysics of cataclysmic variables and related objects", ASP Conf. Ser., eds. J.M. Hameury and J.P. Lasota
dc.identifierhttps://arxiv.org/abs/astro-ph/0410102
dc.identifierhttp://arxiv.org/abs/astro-ph/0410102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8309
dc.subjectAstrophysics
dc.titleThe Turn-off of Classical Novae Observed Through X-rays: Models versus ROSAT Observations of V1974 Cyg
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