Supernovae and Gamma-Ray Burst

Details Supernovae and Gamma-Ray Burst Supernovae and Gamma-Ray Burst

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sngh.conf..110d&link_type=abstract

SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA-RAY EXPERIMENTS The Variable Gamma-Ray Sources: Their Identifications and C

Physics

Scientific paper

We review the observational status of the Supernova/Gamma-Ray Burst connection. Present data suggest that a significant fraction of long-duration GRBs (although not all of them) are associated with bright SNe of type Ib/c. Current estimates of SN and GRB rates yield ratios GRB/SNe-Ibc in the range ~ 0.4% - 3%. In the few SN/GRB associations so far discovered the SN and GRB events appear to be simultaneous events. For the association GRB 060218/SN 2006aj, X and optical observations suggest that the SN and GRB are coeval events within ~ 0.1 days.

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