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在M87连接黑洞和射流的环状积聚结构
Ru-Sen Lu1,2,3, Keiichi Asada4, Thomas P Krichbaum5
1Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, People's Republic of China. rslu@shao.ac.cn.
新事件地平线望远镜拍摄的M87无线电星系显示出一个更大,更厚的环形结构3.5毫米. 这表明黑洞可能有大量的积聚流和风.
科学领域:
- 天体物理学
- 无线电天文学
背景情况:
- 无线电星系M87是研究黑洞积聚和喷气形成的关键对象.
- 2017年之前的事件地平线望远镜 (EHT) 在1.3毫米处的观测显示了其中心黑洞周围的环状结构.
研究的目的:
- 通过使用更高分辨率成像来空间解析M87的紧无线电核心.
- 为了研究不同波长的M87黑洞周围的积聚流和喷射发射区域的结构.
主要方法:
- 2018年获取M87波长3.5mm的高分辨率无线电图像.
- 在黑洞附近观察到的环状结构和排放特征的分析.
主要成果:
- 在3.5毫米的空间分辨率上对M87的紧无线电核心进行成像.
- 一个环状结构的观察,大约比以前的1.3毫米大和厚.
- 有证据表明从喷气发射区域的大量积累流和潜在的风.
结论:
- 在3.5毫米的更大和更厚的环表示显著的增积流与吸收效应,除了透镜发射.
- 观察到的喷气连接到积累流,其更广泛的排放概况表明可能是积累流驱动的风.
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