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

  • Elena Sorokina
  • Sergey Blinnikov
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

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.

Keywords

Light Curve Light Curf Supernova Remnant Reverse Shock Explosion Model 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • Elena Sorokina
    • 1
  • Sergey Blinnikov
    • 2
  1. 1.SAIMoscowRussia
  2. 2.ITEPMoscowRussia

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