最大的莱曼-α星云的中心电源由极化辐射揭示出来
Matthew Hayes1, Claudia Scarlata, Brian Siana
1Université de Toulouse, UPS-OMP, IRAP, Toulouse, France. matthew.hayes@ast.obs-mip.fr
Nature
|August 19, 2011
概括
在 LAB1 块中检测到极化莱曼-α (Lyα) 辐射,显示出环状结构. 这表明Lyα光子起源于宿主星系,并被中性分散.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 银河系的进化 银河系的进化
背景情况:
- 高红移莱曼-α (Lyα) 斑点是罕见的,与密集的宇宙区域相关的发光结构.
- 它们的发光源和形态类似于无线电星系,但仍然不清楚.
- 之前对Lyα发射的偏振研究产生了零检测.
研究的目的:
- 为了研究高红移点斑块中的Lyα发射的起源.
- 为了区分不同的激发机制 (星爆,黑洞积累,超新星,光环气体落入).
- 检测和分析波点LAB1.1.中的极化Lyα辐射.
主要方法:
- 使用先进的望远镜技术对LAB1的观测.
- 测量Lyα发射偏振的方法.
- 分析极化分数作为半径的函数.
主要成果:
- 在LAB1.1的中央区域没有发现可测量的两极分化.
- 在45 kiloparsecs的半径中检测到~20%的极化分数.
- 观察到一个几乎完整的极化环结构.
结论:
- 检测到的极化Lyα辐射与现场光子产生不一致.
- 在星云内的宿主星系中产生了Lyα光子.
- 通过中性的散射是导致观察到的两极分化的机制.
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