发现来自星云的强大的玛射线耀斑
M Tavani1, A Bulgarelli, V Vittorini
1Istituto Nazionale di Astrofisica-Istituto di Astrofisica Spaziale e Fisica Cosmica (INAF-IASF) Roma, via del Fosso del Cavaliere 100, 00133 Roma, Italy. pi.agile@iasf-roma.inaf.it
概括
巨星云 (Crab Nebula) 是一个超新星残留物,它呈现出了由AGILE卫星探测到的意想不到的马射线耀斑. 这些强大而短暂的事件挑战了现有的星云辐射模型.
科学领域:
- 高能天体物理学 高能天体物理学
- 超新星残留物 超新星残留物
- 脉冲星物理学的物理学
背景情况:
- 被脉冲星驱动的星云被认为具有稳定的排放.
- 之前的观测没有表明玛射线输出的显著变化.
研究的目的:
- 报告和分析来自星云的强马射线耀斑的检测.
- 调查这些短暂事件的起源和影响.
主要方法:
- 使用AGILE卫星检测玛射线耀斑 (100 MeV10 GeV).
- 对耀斑流量和时间尺度的分析.
- 讨论从钱德拉和哈勃望远镜获得的互补的X射线和光学数据.
主要成果:
- 2010年9月和2007年10月观察到强烈的马射线耀斑.
- 与静止期相比,马射线流在爆发期间增加了三倍.
- 耀斑的特征表明它起源于靠近脉冲星的地方.
结论:
- 观测到的耀斑挑战了来自星云的星云辐射标准模型.
- 这些发现需要新的模型,包括快速粒子加速,可能通过冲击驱动的等离子体波流.
- 建议加速时间大约为1天.
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