The Edge of a Gamma Ray Burst Afterglow
arXiv:astro-ph/9806183 · doi:10.1046/j.1365-8711.1998.01992.x
Abstract
We discuss the formation of spectral features in the decelerating ejecta of gamma-ray bursts, including the possible effect of inhomogeneities. These should lead to blueshifted and broadened absorption edges and resonant features, especially from H and He. An external neutral ISM could produce detectable H and He, as well as Fe X-ray absorption edges and lines. Hypernova scenarios may be diagnosed by Fe K- and H Ly- emission lines.
M.N.R.A.S., accepted July 16 1998; submitted June 4 1998; latex, 11 pages
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