Evidence of a Long-Duration Component in the Prompt Emission of Short Gamma-Ray Bursts Detected with BeppoSAX
Abstract
A statistical study on the light curves of all the short gamma-ray bursts (GRBs) detected with the Gamma Ray Burst Monitor (GRBM) aboard BeppoSAX is reported. Evidence of a very weak and long-duration component associated with these events in the two 1 s ratemeters of the GRBM (40-700 and >100 keV) is found. It starts a few tens of seconds before the burst and continues for about 30 s after the burst. The overall hardness of this component is comparable to that of the event itself. The detection of a signal before the onset time and the hardness are consistent with an interpretation of the long-duration component in terms of prompt emission associated with short GRBs.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- May 2005
- DOI:
- 10.1086/430759
- arXiv:
- arXiv:astro-ph/0504199
- Bibcode:
- 2005ApJ...625L..17M
- Keywords:
-
- Gamma Rays: Bursts;
- Methods: Statistical;
- Astrophysics
- E-Print:
- 12 pages, 6 figures, accepted for publication in ApJL