发现了与X射线双星相关的非常高能量的玛射线
F Aharonian1, A G Akhperjanian, K-M Aye
1Max-Planck-Institut für Kernphysik, Post Office Box 103980, D-69029 Heidelberg, Germany.
概括
来自微类星 LS 5039 的高能马射线发射被检测到,这表明粒子加速到非常高的能量,类似于活跃的银河系核喷射.
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
- 马射线天文学 马射线天文学
背景情况:
- X射线双星由一个正常恒星围绕一个中子星或黑洞运行.
- 一些被称为微类星的X射线二进制星体,表现出类似活跃银河系核喷射的无线电辐射.
- 众所周知,活跃的银河系核喷气加速粒子到高能量,产生马射线.
研究的目的:
- 为了研究候选微准星LS 5039.9的高能马射线辐射.
- 为了确定微量子星中的粒子是否可以被加速到非常高的能量.
主要方法:
- 使用高能立体系统 (H.E.S.S.) 为了观察. 为了观察.
- 分析100千兆电子伏特以上的马射线信号的数据.
主要成果:
- 从LS 5039.9检测到的马射线辐射的证据.
- 观察到的辐射表明粒子加速到非常高的能量 (>100GeV).
结论:
- 微量子星,如LS 5039,可以加速粒子到非常高的能量.
- 这一发现支持了微类星体和活跃银河系核之间的类比.
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