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扩散的γ射线背景由恒星形成的星系主导
Matt A Roth1, Mark R Krumholz2,3, Roland M Crocker2
1Research School of Astronomy and Astrophysics, The Australian National University, Canberra, Australian Capital Territory, Australia. matt.roth@anu.edu.au.
Nature
|September 16, 2021
概括
只有恒星形成的星系可以解释马射线背景. 一个新的物理模型准确地预测了来自星系宇宙射线相互作用的马射线发射,与费米望远镜的观测相匹配.
科学领域:
- 天体物理学
- 宇宙射线物理
- 银河系天文学
背景情况:
- 费米马射线太空望远镜检测到一个扩散的马射线背景.
- 之前的模型很难限制活跃的星系核和恒星形成的星系的贡献.
研究的目的:
- 开发星系形成过程中的马射线发射的物理模型.
- 确定恒星形成的星系是否可以完全解释同位素的马射线背景.
主要方法:
- 开发了来自宇宙射线与星际介质相互作用的马射线发射的物理模型.
- 通过对当地的星系观测来验证模型.
- 将模型应用于宇宙形成星系群.
主要成果:
- 物理模型与观测到的马射线背景的强度和光谱倾斜度准确匹配.
- 只有恒星形成的星系可以解释完全扩散的同位素马射线背景.
- 该模型不依赖于经验测量.
结论:
- 形成恒星的星系是扩散的银河系外马射线背景的主要贡献者.
- 这项研究为观测到的马射线背景提供了强有力的物理解释.
- 这些发现解决了高能天体物理学中长期存在的问题.
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