TP-29
The external shock model has had much success at reproducing gamma-ray burst afterglows. Economy of hypothesis favors applying this model to the prompt gamma-ray emission as well. The external shock model makes clear predictions about both the time histories and spectral evolution of gamma-ray bursts. Here we test the latter using the observed linear decrease of Epk with respect to energy fluence in several bright gamma-ray bursts. We also confront the spectral indices predicted by the external shock model to occur within three energy bands with those actually observed in BATSE bursts.
Fifth Huntsville Gamma Ray Burst Symposium
Hunsville, Alabama, USA
18-22 October, 1999