Model atmospheres for type I supernovae - Curvature effects

Details Model atmospheres for type I supernovae - Curvature effects Model atmospheres for type I supernovae - Curvature effects

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...184..249l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 184, no. 1-2, Oct. 1987, p. 249-255. Research supported by the Accion Integrad

Astronomy and Astrophysics

Astrophysics

6

Atmospheric Models, Light Curve, Radiative Transfer, Stellar Atmospheres, Supernovae, Dynamic Models, Energy Distribution, Stellar Luminosity, Temperature Profiles

Scientific paper

Type I supernovae are thought to be the result of the thermonuclear explosion of a carbon-oxygen white dwarf in a close binary system. Previous models have shown that the mean free path of photons is of the same order as the size of the configuration and that the curvature effects can no longer be ignored. In this paper the authors propose a simple and accurate generalization of the Eddington relationship and analyze the role played by the curvature of the layers on the radiative transfer.

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