不寻常的马射线爆发GRB 101225A解释为一个小物体落在中子星上
S Campana1, G Lodato, P D'Avanzo
1INAF - Osservatorio Astronomico di Brera, Via E. Bianchi 46, I-23807 Merate, Italy. sergio.campana@brera.inaf.it
Nature
|December 2, 2011
概括
这是一个很棒的节目,这是一个很棒的节目.
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
- 紧的对象研究研究.
背景情况:
- 超大质量黑洞对恒星造成的潮扰乱事件 (TDE) 是众所周知的.
- 涉及小物体和恒星,或紧物体的类似过程较少被探索.
- 彗星对中子星的积聚以前被认为是玛射线发射的来源.
研究的目的:
- 为了解释马射线爆发GRB 101225A的不寻常特征.
- 研究涉及小物体和紧的恒星残骸的潮破坏事件的可能性.
- 探索对中子星周围的小物体捕获和形成的影响.
主要方法:
- 对GRB 101225A.的观测数据的分析.
- 潮破坏事件的理论建模.
- 与已知的天体物理现象进行比较.
主要成果:
- GRB 101225A的特殊特征与银河系中子星周围的一个小物体的潮破坏事件一致.
- 这一事件表明,小物体可能比以前认为的更频繁地被紧的残骸所捕获.
- 另一个解释涉及与玛射线爆发相关的奇特超新星.
结论:
- 中子星对小天体的潮干扰可以解释不寻常的马射线爆发.
- 紧的恒星残留物捕获小物体的频率可能被低估.
- 需要进一步的研究,以了解在毫秒脉冲星周围的小物体形成.
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