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低水平的银河系外背景光,由来自Blazar的马射线揭示出来
F Aharonian1, A G Akhperjanian, A R Bazer-Bachi
1Max-Planck-Institut für Kernphysik, PO Box 103980, D 69029 Heidelberg, Germany.
Nature
|April 21, 2006
概括
研究人员使用Blazar马射线光谱研究了扩散的银河系外背景光. 研究结果表明,来自银河系的恒星光占主导地位,排除了早期的显著贡献.
科学领域:
- 天文学和天体物理学
- 宇宙微波背景辐射宇宙微波背景辐射
背景情况:
- 扩散的银河系外背景光 (DEBL) 是整个宇宙历史上来自银河系的星光.
- DEBL可能包括来自宇宙第一个恒星的贡献,这些恒星早于星系形成.
- 直接测量DEBL是具有挑战性的,因为前景光,像生肖的光.
研究的目的:
- 为了限制分散的银河系外背景光的组成.
- 调查早期恒星对DEBL的贡献.
- 为了评估星际空间对马射线的透明度.
主要方法:
- 分析来自遥远的闪电星 (H 2356-309和1ES 1101-232) 的马射线光谱.
- 研究由光子与DEBL相互作用引起的马射线光谱中的吸收特征.
- 使用Blazar光谱来设置DEBL强度的上限.
主要成果:
- 在红移 z = 0.165 和 z = 0.186.6 时检测到来自布莱扎的马射线辐射.
- 观察到来自这些闪电星的意外硬的马射线光谱.
- 建立了光学/近红外DEBL的上限,靠近来自分辨率高的星系的集成光.
结论:
- 扩散的银河系外背景光被来自银河系的直接恒星光强烈主导.
- 第一颗星对DEBL的重大贡献被排除在外.
- 星际空间对马射线的透明度比以前所认为的要大.
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