UV Light Curves of Thermonuclear Supernovae

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dc.creatorBlinnikov, S. I.
dc.creatorSorokina, E. I.
dc.date2000-03-17
dc.date.accessioned2026-07-07T01:52:47Z
dc.date.available2026-07-07T01:52:47Z
dc.descriptionUltraviolet light curves are calculated for several thermonuclear supernova models using a multifrequency radiation hydrodynamic code. It is found that Chandrasekhar-mass models produce very similar light curves both for detonation and deflagration. Sub-Chandrasekhar-mass models essentially differ from ``normal'' Chandrasekhar ones regarding behaviour of their UV fluxes. Differences in absolute brightness and in shape of light curves of thermonuclear supernovae could be detectable up to 300 Mpc with modern UV space telescopes.
dc.description3 pages, 2 figures, aa.cls LaTeX, accepted by Astron.Asrophys.Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/0003247
dc.identifierhttp://arxiv.org/abs/astro-ph/0003247
dc.identifierAstron. Astrophys. v. 356, p. L30-L32 (2000)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/736
dc.subjectAstrophysics
dc.titleUV Light Curves of Thermonuclear Supernovae
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