Temporal properties of short GRBs
arXiv:astro-ph/0103192 · doi:10.1046/j.1365-8711.2002.05136.x
Abstract
We analyze a sample of bright short bursts from the BATSE 4B-catalog and find that many short bursts are highly variable (, where is the shortest pulse duration and T is the burst duration). This indicates that it is unlikely that short bursts are produced by external shocks. We also analyze the available (first 1-2 seconds) high resolution (TTE) data of some of the long bursts. We find that variability on a 10ms time-scale is common in long bursts. This result shows that some long bursts are even more variable than it was thought before ( )
7 pages, 9 figures, accepted for publication by MNRAS
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