The BATSE View of the Transition from GRB to Afterglow

Details The BATSE View of the Transition from GRB to Afterglow The BATSE View of the Transition from GRB to Afterglow

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312...29g&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

Scientific paper

A careful examination of the BATSE data suggests that afterglow emission, presumably due to a forward external shock, may initially peak in γ-rays and may overlap in time with the prompt Gamma-Ray Burst (GRB) emission. We discuss the properties of extended emission tails observed in BATSE GRBs and the possibility that the afterglow flux may intially be variable.

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