在微类星星Cygnus X-3中极端粒子加速
M Tavani1, A Bulgarelli, G Piano
1INAF-IASF Roma, Via del Fosso del Cavaliere 100, I-00133 Roma, Italy. pi.agile@iasf-roma.inaf.it
Nature
|November 26, 2009
概括
天文学家发现了来自微类星天X-3的高能马射线耀斑,为这些系统中的粒子加速提供了证据. 这一发现有助于解释微量子星中能量喷气形成背后的机制.
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
- X射线天文学X射线天文学
背景情况:
- 微量子星,银河系的双星系统,产生相对论喷射和无线电耀斑.
- 在微量子星中,关于千兆电子伏粒子加速的证据很少,这使得喷射能量化机制不清楚.
研究的目的:
- 为了研究来自微类星天X-3的马射线辐射.
- 探索玛射线耀斑,光谱状态和微量子星中的喷气喷射之间的关系.
主要方法:
- 来自天X-3的100 MeV以上的马射线耀斑的观测.
- 分析玛射线耀斑和无线电/X射线发射状态之间的时间相关性.
主要成果:
- 从天X-3探测到四个马射线耀斑.
- 在玛射线耀斑和过渡光谱状态之间发现了时间相关性.
- 在两个实例中,粒子加速先于射电喷射喷射,这表明喷射形成过程中能量粒子的产生.
结论:
- 微夸星可以将粒子加速到非常高的能量,比静止状态高数千倍.
- 这项研究为微量子星中千兆电子伏粒子加速提供了系统的证据.
- 微量子星中喷气形成与高能粒子的产生有关.
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