Temporal and Spectral Characteristics of Short Bursts from the Soft Gamma Repeaters 1806-20 and 1900+14
Abstract
We study the temporal and coarse spectral properties of 268 bursts from SGR 1806-20 and 679 bursts from SGR 1900+14, all observed with the Rossi X-Ray Timing Explorer/Proportional Counter Array. Hardness ratios and temporal parameters, such as T90 durations and τ90 emission times are determined for these bursts. We find a lognormal distribution of burst durations, ranging over more than 2 orders of magnitude: T90 ~ 10-2 to >~1 s, with a peak at ~0.1 s. The burst light curves tend to be asymmetrical, with more than half of all events showing rise times tr < 0.3 T90. We find that there exists a correlation between the duration and fluence of bursts from both sources. We also find a significant anticorrelation between hardness ratio and fluence for SGR 1806-20 bursts and a marginal anticorrelation for SGR 1900+14 events. Finally, we discuss possible physical implications of these results within the framework of the magnetar model.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 2001
- DOI:
- 10.1086/322463
- arXiv:
- arXiv:astro-ph/0105110
- Bibcode:
- 2001ApJ...558..228G
- Keywords:
-
- Gamma Rays: Bursts;
- stars: individual (SGR 1806-20;
- SGR 1900+14);
- X-Rays: Bursts;
- Astrophysics
- E-Print:
- 24 pages, 11 figures, accepted for publication in ApJ