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银河系核风中的冷气体
Enrico M Di Teodoro1,2,3, N M McClure-Griffiths4, Felix J Lockman5
1Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA. editeodoro@jhu.edu.
Nature
|August 21, 2020
概括
科学家发现冰冷,密集的分子气体从银河系流出
科学领域:
- 天体物理学
- 银河系动力学
- 星际介质
背景情况:
- 银河中心经历了来自射手座A*和恒星反的高能量过程.
- 这些过程驱动银河系风,从银河系盘中驱逐物质和能量.
- 观察到的外流气体包括热电离,热电离和冷原子相.
研究的目的:
- 在银河系的星系风中研究冷,密集的分子气体的存在和特性.
- 了解此前未被观察到的气相的起源和影响.
主要方法:
- 高分辨率的分子气体外流观测.
- 分析冷气云的形态和动力学.
- 与核风中的原子云有关.
主要成果:
- 直接观察从银河系中心流出的冷密分子气体.
- 分子气体云与更温暖的外流介质混合并可能被破坏.
- 分子外流的质量很大,可能会影响中心恒星的形成.
结论:
- 在银河系风中发现冷分子气体挑战了现有的模型.
- 目前的射手座A*活动和中心恒星形成都不能完全解释这种气体的存在.
- 在星系进化和恒星形成中起到至关重要的作用.
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