来自无线电星系M87的特拉电子伏特马射线的快速变化
F Aharonian1, A G Akhperjanian, A R Bazer-Bachi
1Max-Planck-Institut für Kernphysik, Post Office Box 103980, D 69029 Heidelberg, Germany.
概括
来自无线电星系M87的特拉电子伏特 (TeV) 马射线流的快速变化表明其黑洞附近有一个紧的发射区域. 这一发现排除了其他生产地点,并证实了超银河系的TeV马射线来源超出了布莱扎.
科学领域:
- 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
- 银河系外的天文学.
背景情况:
- 无线电星系M87是高能现象的来源.
- 了解特拉电子伏特 (TeV) 马射线的起源对天体物理学至关重要.
- 以前的观测表明,来自银河系外的源头的马射线流变化较慢.
研究的目的:
- 来自M87.7.的TeV马射线流的快速变化的检测报告.
- 为了研究这些快速变化的影响,排放区域大小.
- 为了限制超银河系源中的马射线产生模型.
主要方法:
- 来自M87.87的TeV马射线辐射的观测和分析.
- 对玛射线流量变化的时间尺度分析.
- 将变化时间尺度与其他波段和理论模型进行比较.
主要成果:
- 检测来自M87.7的TeV马射线流中的快速 (日间) 变化.
- 这些变化大约是以前在其他波段观察到的速度的10倍.
- 快速的变化意味着一个非常紧的辐射区域,与M87中心黑洞的施瓦茨希尔德半径相当.
结论:
- 紧的发射区域排除了几个拟议的马射线生产地点和过程.
- 这些发现证实,TeV马射线可以从除了布莱扎之外的银河系外来源发出的.
- 这支持了TeV马射线辐射的存在,这些辐射来自没有相对论向观测者的喷射源.
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