在原星团中的活跃星系周围的宇宙网络的气体丝
H Umehata1,2, M Fumagalli3,4,5, I Smail3
1RIKEN Cluster for Pioneering Research, 2-1 Hirosawa, Wako-shi, Saitama 351-0198, Japan. hideki.umehata@riken.jp.
天文学家在早期宇宙中检测到来自连接星系的气体丝的微弱紫外线. 这些结构跨越一个兆帕塞克, 提供了关于星系和黑洞形成的关键见解.
科学领域:
- 宇宙学
- 天体物理学
- 星系的形成
背景情况:
- 太空学模拟预测一个星系间气体丝的宇宙网络.
- 由于它们的微弱发射, 观测这些丝是具有挑战性的.
- 这些细丝被认为对星系进化至关重要.
研究的目的:
- 检测和描述来自星际气体丝的辐射.
- 测试宇宙网络结构及其在星系形成中的作用.
- 调查电离辐射发电源的发电.
主要方法:
- 检测休息紫外线莱曼α辐射.
- 观察重点是SSA22原团在红移z = 3.1时.
- 在星系之间绘制延伸的丝状结构.
主要成果:
- 成功检测了来自多个细丝的莱曼α排放.
- 星系之间有超过1兆帕塞克的线程.
- 星系内有强烈的恒星形成和活跃的超大质量黑洞.
结论:
- 观察到的莱曼α辐射是由嵌入的星系的电离辐射驱动的.
- 这些发现支持有线气体为星系和黑洞增长提供燃料的理论.
- 这项研究提供了宇宙网络在结构形成中的作用的观察证据.
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