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Explosions inside Ejecta and Most Luminous Supernovae

Authors
  • Blinnikov, S. I.
Type
Published Article
Publication Date
Dec 28, 2008
Submission Date
Dec 28, 2008
Identifiers
DOI: 10.1063/1.2943580
Source
arXiv
License
Yellow
External links

Abstract

The extremely luminous supernova SN2006gy is explained in the same way as other SNIIn events: light is produced by a radiative shock propagating in a dense circumstellar envelope formed by a previous weak explosion. The problems in the theory and observations of multiple-explosion SNe IIn are briefly reviewed.

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