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在银河系中心的超大质量黑洞候选物体中的事件视界尺度结构
Sheperd S Doeleman1, Jonathan Weintroub, Alan E E Rogers
1Massachusetts Institute of Technology (MIT) Haystack Observatory, Off Route 40, Westford, Massachusetts 01886, USA. sdoeleman@haystack.mit.edu
Nature
|September 5, 2008
概括
天文学家在1.3毫米处观测了射手座A*,揭示了它的内在直径比黑洞事件地平线的预期要小. 这表明辐射源于周围的积累流,而不是黑洞本身.
科学领域:
- 天文学和天体物理学
- 黑洞物理学 黑洞物理学
- 银河系的核心
背景情况:
- 超大质量黑洞通过增加物质来为活跃的银河系核提供动力.
- 射手座A* (Sgr A*) 是距离银河系中心最近的超大质量黑洞.
- 了解Sgr A*附近的结构对于理解强重力下的积累物理至关重要.
研究的目的:
- 为了了解射手座A*周围最内在的积累流的结构.
- 确定Sgr A*在波长为1.3mm的内在尺寸.
- 调查Sgr A*的排放来源.
主要方法:
- 在波长为1.3毫米的射手座A*进行了高分辨率无线电观测.
- 分析了观察到的数据,以确定Sgr A*的内在直径.
- 将观察到的尺寸与黑洞事件视界预期的表面尺寸进行比较.
主要成果:
- 射手座A*的内在直径被测得为37±+16±-10) 微弧秒.
- 这种测量的大小小于黑洞事件视界预测的表面大小.
- 这些发现挑战了假设辐射直接集中在黑洞上的假设.
结论:
- 射手座A*辐射的大部分可能来自周围的积聚流,而不是黑洞本身.
- 这项研究为超大质量黑洞附近的积累过程提供了新的约束.
- 需要进一步的研究才能充分了解Sgr A*的排放机制.
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