English

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 (δtmin/T1\delta t_{min}/T\ll 1, where δtmin\delta t_{min} 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 (δtmin/T104103\delta t_{min}/T\approx 10^{-4}-10^{-3} )

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

R2 v1 2026-07-22T07:56:26.925Z