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Tests for Supernova Explosion Models: from Light Curves to X-ray Emission of Supernova Remnants

Published online by Cambridge University Press:  19 September 2016

Elena Sorokina  and
Sergey Blinnikov
Elena Sorokina
Affiliation:
SAI, Universitetskij pr. 13, 119992 Moscow, Russia;sorokina@sai.msu.su
Sergey Blinnikov
Affiliation:
ITEP, B. Cheremushkinskaya 25, 117218 Moscow, Russia;blinn@sai.msu.su

Summary

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The successful theoretical supernova explosion models should be able to explain any features of the emission from supernovae at any evolutionary stage. We check several models from two different points of view. With the multi-frequency radiation hydro code STELLA we calculate gamma-ray, bolometric and broad-band UBVI light curves. Then we use the same models to calculate the emission from young supernova remnants. Here we present new plots for gamma-ray luminosity from several SN Ia models and recomputations of bolometric and UBVRI light curves of model 13C for SN 1993J.

Type
Part IV Supernovae: Models
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 269 - 274
Copyright
Copyright © Springer-Verlag 2005

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