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来自磁星SGR 1806-20的一个巨大的马射线耀斑
D M Palmer1, S Barthelmy, N Gehrels
1Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA. palmer@lanl.gov
Nature
|April 29, 2005
概括
软马射线重复器 (SGR) 是磁器,发射强大的X射线爆发. 来自SGR 1806-20的巨型耀斑释放了2 x 10^46 erg,可能是由于磁场重新配置.
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
- 中子星物理学 中子星物理学
背景情况:
- 磁星是中子星,具有超强的磁场 (约. 10^15 G) 的数量.
- 软马射线重复器 (SGR) 和异常X射线脉冲星属于磁星类.
- 在SGR中,偶尔会出现爆发和极为罕见的巨型火焰.
研究的目的:
- 报告和分析来自磁星SGR 1806-20的巨型耀斑事件.
- 为了描述所观察到的耀斑的能量输出和潜在原因.
主要方法:
- 来自SGR 1806-20的X射线辐射数据的观察和分析.
- 巨型耀斑事件的能量计算.
主要成果:
- 2004年12月27日,从SGR 1806-20观测到一个巨大的耀斑.
- 耀斑的同otropic 能量达到2 x 10^46 erg,明显超过之前的巨型耀斑.
- 能量释放归因于灾难性的磁场重新配置.
结论:
- 观测到的巨型耀斑为磁星能量释放机制提供了洞察力.
- 这样的事件,如果从银河系外的距离观察到,可以被归类为短,硬的马射线爆发.
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