一个典型的恒星形成星系的形成和组装在红移z大约3的典型恒星形成星系
Daniel P Stark1, A Mark Swinbank, Richard S Ellis
1Department of Astronomy, California Institute of Technology, Pasadena, California 91125, USA. dps@astro.caltech.edu
Nature
|October 10, 2008
概括
大爆炸后20亿到30亿年观察到的银河系盘表明,气体积聚,而不是合并,推动了银河系的增长. 这项研究证实了典型星系的这一点,揭示了旋转气盘中高效的恒星形成.
科学领域:
- 银河系的宇宙进化过程
- 银河系的形成和演变.
- 天体物理学 天体物理学
背景情况:
- 早期的星系 (大爆炸后的2-3年) 显示出大型的旋转盘,这意味着气体在合并过程中积聚.
- 以前的研究仅限于发光星系,可能不代表典型的星系组合.
- 高分辨率的观测对于理解较弱光度星系的生长至关重要.
研究的目的:
- 研究典型的恒星形成星系在高红移 (z = 3.07) 的生长机制.
- 解决这些星系中气体和恒星形成的空间结构和动态.
- 为了测试气体积聚在银河系增长中占据主导地位的假设.
主要方法:
- 高分辨率观测一个典型的恒星形成星系在z = 3.07.
- 对分子气体含量和恒星形成速度的分析.
- 详细检查银河系的速度场和结构.
主要成果:
- 在一个典型的星系中观察一个紧的,有序的旋转源.
- 在这个源中,分子气体高效地转化为恒星.
- 形成球形凸起的证据,类似于今天的螺旋星系.
结论:
- 气体积聚是典型星系生长的一个重要机制,即使在早期的宇宙时代.
- 观察到的旋转表明,主要的合并并不是这种星系质量组合的主要驱动因素.
- 这些发现支持像银河系这样的星系通过连续的气体流入积累质量的模型.
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