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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
不寻常的γ射线爆发GRB 101225A来自星/中子星合并,红移0.33
C C Thöne1, A de Ugarte Postigo, C L Fryer
1IAA - CSIC, Glorieta de la Astronomía s/n, 18008 Granada, Spain. cthoene@iaa.es
Nature
|December 2, 2011
概括
异常长的马射线爆发 (GRB) 101225A呈现出长期存在的辐射,随后是热X射线短暂和光学超新星. 星与中子星的合并被认为是原始事件.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 恒星进化中的恒星演变
背景情况:
- 长马射线爆发 (GRBs) 与巨大的恒星死亡和超新星有关.
- GRB涉及超相对论喷射,通过同步子辐射产生非热辐射.
- 了解GRB的祖先和发射机制对于天体物理学至关重要.
研究的目的:
- 为了分析长玛射线爆发GRB 101225A.的独特特征.
- 调查这种不寻常的GRB事件的发射机制和祖先.
- 为了确定GRB 101225A的红移和宿主星系属性.
主要方法:
- 观测和分析GRB 101225A的马射线,X射线和光学辐射.
- 将光谱能量分布和光曲线与GRB超新星模板相匹配,以估计红移.
- 将辐射建模为一个膨胀,冷却的黑体和随后的超新星.
主要成果:
- GRB 101225A显示出异常长寿命的马射线辐射.
- 观察到一个明亮的X射线瞬态与热热组件和一个不寻常的光学对应物.
- 光学发射演变为一个冷却的黑体,随后是微弱的超新星组成部分,估计红移为z = 0.33.
结论:
- 一个被提议的祖先是星与中子星的合并,导致GRB类喷气体被弹出的物质热化.
- 另一个解释是,一个小物体聚集在银河中子星上.
- 观察到的现象挑战了传统的GRB模型,表明了不同的祖先场景.
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