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Cryogenic Liquid Jets for High Repetition Rate Discovery Science
Published on: May 9, 2020
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高红移星系周围的冷分子气体的大流库
E Falgarone1, M A Zwaan2, B Godard1
1LERMA/LRA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Université Paris 06, Ecole normale supérieure, 75005 Paris, France.
Nature
|August 17, 2017
概括
这些星系利用星系风来维持流,延长它们的星系爆发阶段. 这些风将气体转化为储备,但需要通过合并或积聚增加质量以形成燃料恒星.
科学领域:
- 天文学与天体物理学
- 宇宙进化
- 星系的形成和演变
背景情况:
- 这些星系是强大的宇宙引擎,
- 维持这些速度需要大量的冷分子气体,尽管反过程.
- 甲基 (CH+) 是非平衡气体条件的标志物,表明能量消散.
研究的目的:
- 为了研究星系反在星系爆炸中的作用.
- 探测星系内外气体的物理条件.
- 了解反,流和星系增长之间的相互作用.
主要方法:
- 在红移2.5的透镜星系中检测CH+ (J=1-0) 发射和吸收线.
- 对线性质 (宽度,临界密度) 的分析,以推断气体条件和来源.
- 气体储备和大规模流出率的建模.
主要成果:
- 射线表示由银河系风驱动的强冲击波.
- 气吸收线显示出流,凉爽的气体储延伸到星爆核心之外.
- 银河系的风能维持流, 形成多相水库,
结论:
- 星系反,加上流和重力, 延长了星爆阶段.
- 为了保持高的恒星形成率,需要额外的质量输入,可能来自合并或冷流.
- 这项研究提供了有关早期宇宙中强烈恒星形成的机制的见解.
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