一个X射线烟延伸在银河系中心上下数百个帕塞克
G Ponti1,2, F Hofmann3, E Churazov4,5
1Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany. gabriele.ponti@inaf.it.
Nature
|March 22, 2019
概括
银河系中心的外流会产生X射线结构,
科学领域:
- 天文学与天体物理学
- 银河系动力学
背景情况:
- 银河系中心的外流对银河系结构有很大影响.
- 之前的观测发现了双极叶,费米气泡和银河系中心叶,
研究的目的:
- 报告和描述连接银河中心与费米泡的突出X射线结构.
- 提出这些结构作为能源和大众运输的"烟".
主要方法:
- 来自ROSAT全天空调查的X射线数据的分析.
- 在银河平面上方和下方的中间尺度 (数百帕塞克) 观测X射线结构.
主要成果:
- 在中间尺度 (数百帕塞克) 上发现了突出的X射线结构.
- 这些结构似乎将银河系中心区域与更大的费米泡连接起来.
- 证据表明这些结构作为能量和质量的运输道.
结论:
- 已发现的X射线结构被称为银河中心"烟", 对于能量和质量的传输至关重要.
- 这些"烟"将银河系中心的周期性能量事件与费米泡的底部联系起来.
- 银河系中心的外流在形成大规模银河系结构中起着至关重要的作用.
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