GRB Environment Deduced from Afterglow Emission

Details GRB Environment Deduced from Afterglow Emission GRB Environment Deduced from Afterglow Emission

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..34k&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

I will provide an overview of our understanding of the environment
withinabout one parsec of gamma-ray bursts. Evidence for and against the
presenceof a stratified medium carved out by theprogenitor star's wind
will be described.

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