来自星云的马射线耀斑
A A Abdo1, M Ackermann, M Ajello
1National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA.
概括
星云在2009年和2010年经历了两次强大的马射线耀斑,表明了peta-electron-volt电子的存在. 这些能量事件挑战了天体物理源中粒子加速的当前理论.
科学领域:
- 高能天体物理学 高能天体物理学
- 粒子物理学的粒子物理学.
- 观测天文学是一种观测天文学.
背景情况:
- 星云由一个年轻,充满活力的脉冲星提供动力.
- 已知脉冲星会发射高能辐射.
研究的目的:
- 描述和分析来自星云的两个不同的马射线耀斑.
- 调查导致这些火焰的粒子的起源和能量.
主要方法:
- 使用费米马射线太空望远镜上的大面积望远镜 (LAT) 检测马射线耀斑.
- 分析马射线的流量和爆发的持续时间.
主要成果:
- 在2009年2月 (16天) 和2010年9月 (4天) 观测到两次马射线耀斑.
- 在爆发期间,马射线流量增加了四倍和六倍.
- 耀斑表明,在一个紧的区域 (<1.4 × 10−2 帕塞克) 中,来自 peta-electron-volt 电子的辐射.
结论:
- 观测到的耀斑与有史以来与离散天文源相关的最高能量的粒子有关.
- 极端能量挑战了现有的粒子加速机制模型.
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