Mass Loss Environment of Long GRBs and Core Collapse SNe

Details Mass Loss Environment of Long GRBs and Core Collapse SNe Mass Loss Environment of Long GRBs and Core Collapse SNe

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..14c&link_type=abstract

Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 8, 2006, Kavli Institute for Theoretical Physics,

Physics

Scientific paper

The environment of core collapse supernovae is probed by their radio andX-ray emission. The various supernova types(IIP, IIL, IIb, IIn, Ib/c) have characteristic radio properties; thedifferences can be attributed to the mass loss density and the velocity ofthe interaction region. The Type Ic SN 1998bw, associated with GRB980425, fits into this scheme, although with a high velocity. Theafterglows of long GRBs are more difficult to reconcile with the expectedmass loss environment.

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