English

New results on the temporal structure of GRBs

Astrophysics 2009-11-06 v1

Abstract

We analyze the temporal structure of long ((T_{90}>2sec)) and short ((T_{90}<2sec)) BATSE bursts. We find that: (i) In many short bursts (\delta t_{min}/T\ll 1) (where (\delta t_{min}) is the shortest pulse). This indicates that short bursts arise, like long ones, in internal shocks. (ii) In long bursts there is an excess of long intervals between pulses (relative to a lognormal distribution). This excess can be explained by the existence of \emph{quiescent times}, long periods with no signal above the background that arise, most likely, from periods with no source activity. The lognormal distribution of the intervals (excluding the \emph{quiescent times}) is similar and correlated with the distribution of the pulses width, in agreement with the predictions of the internal shock model.

Keywords

Cite

@article{arxiv.astro-ph/0103011,
  title  = {New results on the temporal structure of GRBs},
  author = {E. Nakar and T. Piran},
  journal= {arXiv preprint arXiv:astro-ph/0103011},
  year   = {2009}
}

Comments

3 pages 2 figures, poster presented at the ROME GRB meeting