Temporal properties of short GRBs
Astrophysics
2009-11-06 v2
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 ( )
Keywords
Cite
@article{arxiv.astro-ph/0103192,
title = {Temporal properties of short GRBs},
author = {Ehud Nakar and Tsvi Piran},
journal= {arXiv preprint arXiv:astro-ph/0103192},
year = {2009}
}
Comments
7 pages, 9 figures, accepted for publication by MNRAS