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连接到M87中旋转的黑洞的喷射喷嘴
Yuzhu Cui1,2,3,4, Kazuhiro Hada5,6, Tomohisa Kawashima7
1Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou, China. yuzhu_cui77@163.com.
Nature
|September 27, 2023
概括
研究人员分析了22年来对M87星系的无线电观测. 他们在飞机上发现了11年的时间
科学领域:
- 天体物理学
- 无线电天文学
- 黑洞物理
背景情况:
- 无线电星系M87为研究超大质量黑洞和相对论喷流提供了一个独特的实验室.
- 之前的观测表明喷气孔的开放角度很大,并可能与8-10年的准周期性有关.
- 事件地平线望远镜解析了中央无线电源, 显示了一个不对称的环结构.
研究的目的:
- 在M87中观察到的横向喷气转移的起源.
- 分析长期无线电观测以确定喷气的位置的周期性变化.
- 了解积聚盘与黑洞相互作用的动态.
主要方法:
- 对M87的22年无线电观测数据的分析.
- 时间序列分析以检测喷气的位置角度的周期性变化.
- 建模以推断对观察到的喷气行为负责的物理过程.
主要成果:
- 在喷气式飞机的位置角度变化中确定了11年的时间.
- 观察到的喷气前行与旋转的黑洞是一致的.
- 这些发现表明Lense-Thirring前置错位的积累盘.
结论:
- M87的11年喷气前行可能是由旋转的黑洞和错位的积累盘造成的.
- 喷射前行可能是活跃星系核中常见的现象,尽管往往难以检测.
- 这项研究为黑洞,积聚盘和相对论喷流之间的复杂关系提供了重要的见解.
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