短马射线爆发的起源与当前的恒星形成无关
S D Barthelmy1, G Chincarini, D N Burrows
1NASA/Goddard Space Flight Center Greenbelt, Maryland 20771, USA. scott@lheamail.gsfc.nasa.gov
Nature
|December 16, 2005
概括
短马射线爆发 (GRBs) 并不是来自超新星. 新证据表明,这些宇宙爆炸可能源于中子星或黑洞-中子星双星的合并.
科学领域:
- 天体物理学 天体物理学
- 宇宙爆炸,宇宙爆炸.
- 高能天文学 高能天文学
背景情况:
- 两个短的马射线爆发 (GRBs) 与检测到的后照有不清楚的宿主星系起源.
- 一个短暂的GRB发生在形成恒星的矮星系中,另一个发生在可能的圆星系中.
研究的目的:
- 为了确定短玛射线爆发 (GRBs) 的起源.
- 为了研究宿主星系属性和短GRBs的祖先系统.
主要方法:
- 短时间GRB 050724.4的X射线定位.
- 分析玛射线和X射线的光照后光特性.
- 与以前的GRB观测和理论模型进行比较.
主要成果:
- GRB 050724的X射线余照被定位在一个圆星系的中心外,红移z = 0.258.
- 圆星系的恒星形成率较低,这使得GRB 050724.4的超新星起源不太可能.
- 短GRB的同位素能量明显低于长GRB的同位素能量.
结论:
- 短GRB不太可能起源于超新星爆炸.
- 二进制中子星或中子星-黑洞对的凝聚是短GRB的可能祖先.
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