Explosions inside Ejecta and Most Luminous Supernovae
Astrophysics
2010-12-13 v1
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.
Keywords
Cite
@article{arxiv.0812.4802,
title = {Explosions inside Ejecta and Most Luminous Supernovae},
author = {S. I. Blinnikov},
journal= {arXiv preprint arXiv:0812.4802},
year = {2010}
}
Comments
9 pages, 6 figures, LateX aipproc.cls. A bit more details and color added to Fig.3. The 10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG07), Sapporo, Japan, December 2007