UV Light Curves of Thermonuclear Supernovae

Details UV Light Curves of Thermonuclear Supernovae UV Light Curves of Thermonuclear Supernovae

2000-03-17

arxiv.org/abs/astro-ph/0003247v1

Astron. Astrophys. v. 356, p. L30-L32 (2000)

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figures, aa.cls LaTeX, accepted by Astron.Asrophys.Letters

Scientific paper

Ultraviolet 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.

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