从银河系中心山脊发现了非常高能量的马射线
F Aharonian1, A G Akhperjanian, A R Bazer-Bachi
1Max-Planck Institut für Kernphysik, PO Box 103980, D 69029 Heidelberg, Germany.
Nature
|February 10, 2006
概括
银河系宇宙射线起源于超新星残余物. 观测显示了与分子云相关的非常高能量的马射线辐射,这表明质子和原子核是源头.
科学领域:
- 天体物理学 天体物理学
- 高能天文学 高能天文学
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 银河系宇宙射线 (高达10^15 eV) 的起源尚未完全理解.
- 超新星残留物是假设的来源,而马射线观测是研究宇宙射线加速和传播的关键.
研究的目的:
- 为了调查银河系宇宙射线的来源.
- 为了分析银河系中部区域的非常高能量的马射线辐射.
主要方法:
- 对扩展的非常高能 (> 10^11 eV) 马射线辐射的观测.
- 与银河系中心 (200 帕塞克) 的巨大分子云进行空间相关性分析.
主要成果:
- 检测到一个非常高能量的马射线辐射的扩展区域.
- 这种辐射在空间上与一个由巨型分子云组成的复合物相关.
- 马射线光谱的硬度表明宇宙射线是质子和核,而不是电子.
结论:
- 观测到的马射线辐射可能源于分子云内的宇宙射线相互作用.
- 这些宇宙射线的能量来源可能是大约10^4年前的一次超新星爆炸.
- 这项研究提供了支持超新星残骸作为银河系宇宙射线加速器的证据.
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