Temporal and spectral characteristics of short bursts from the soft gamma repeaters 1806-20 and 1900+14

被引:77
作者
Gögüs, E [1 ]
Kouveliotou, C
Woods, PM
Thompson, C
Duncan, RC
Briggs, MS
机构
[1] Univ Alabama, Dept Phys, Huntsville, AL 35899 USA
[2] NASA, Marshall Space Flight Ctr, Huntsville, AL 35805 USA
[3] Univ Space Res Assoc, Washington, DC USA
[4] Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
[5] Univ Texas, Dept Astron, Austin, TX 78712 USA
关键词
gamma rays : bursts; stars; individual; (SGR; 1806-20; SGR; 1900+14); X-rays : bursts;
D O I
10.1086/322463
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 T-90 durations and iota (90) emission times are determined for these bursts. We find a lognormal distribution of burst durations, ranging over more than 2 orders of magnitude: T-90 similar to 10(-2) to greater than or similar to 1 s, with a peak at similar to 0.1 s. The burst light curves tend to be asymmetrical, with more than half of all events showing rise times t(r) < 0.3 T-90. 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.
引用
收藏
页码:228 / 236
页数:9
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