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银河系中心黑洞周围的一个凉爽的积聚盘
Elena M Murchikova1,2, E Sterl Phinney3, Anna Pancoast4
1Institute for Advanced Study, Princeton, NJ, USA. lena@ias.edu.
Nature
|June 7, 2019
概括
天文学家在银河系中部超大质量黑洞"射手座A"附近发现了一颗旋转的离子气体盘. 这一发现使用H30α光谱线,揭示了以前没有被观察所限制的气体特性.
科学领域:
- 天体物理学与天文学
- 黑洞研究
- 银河系中心的气体动力学
背景情况:
- 银河系的中心超大质量黑洞,射手座A*,质量为4×106太阳质量.
- 射手座A*周围有热气和冷气储备, 但黑洞积聚区的冷气质量仍然不受限制.
- 重组光谱线为检测这种较冷气体提供了潜在的方法.
研究的目的:
- 图像和描述冷,离子化的气体盘周围的射手座A*.
- 限制这种气体成分的质量和密度.
- 研究超大质量黑洞附近气体的物理过程.
主要方法:
- 使用1.3毫米射电天文学观察H30α重组线.
- 拍摄了射手座A*的2×10^4施瓦茨希尔德半径内的气体盘.
- 分析了双峰排放线形状和空间分布以推断气体特性.
主要成果:
- 成功拍摄了一个围绕射手座A*旋转的10^4克尔文离子气盘.
- 该磁盘呈现出双峰的H30α发射线,其全速线宽为2200公里/秒.
- 观察到的辐射强于预期,表明H30α过渡的质量增强.
结论:
- 这些观测显示出一个旋转的气体盘,估计质量为10^-5到10^-4太阳质量,密度为10^5到10^6cm^-3.
- 红移和蓝移的发射元件的空间位移表明磁盘内的旋转.
- 增强的H30α辐射表明巨星放大,这是了解黑洞附近气体物理的一个重要发现.
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