Where are the soft gamma-ray repeaters?

被引：0
|
作者：
Kaplan, DL [1 ]
机构：
[1] CALTECH, Dept Astron, Pasadena, CA 91125 USA
来源：
NEUTRON STARS IN SUPERNOVA REMNANTS | 2002年 / 271卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Using observations of the Soft Gamma-Ray Repeaters (SGRs) SGR 1900+14, SGR 1806-20, and SGR 0526-66 with the Chandra Xray Observatory and other facilities, we find that only SGR 0526-66 is plausibly associated with a supernova remnant. However, the locations of all three SGRs are consistent with regions of massive star formation.
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页码：266 / 269
页数：4
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