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窒息是关闭星系恒星形成的主要机制
Y Peng1, R Maiolino1, R Cochrane2
11] Cavendish Laboratory, University of Cambridge, 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UK [2] Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK.
Nature
|May 15, 2015
概括
星系火,即停止恒星形成,主要是由窒息引起的,在这种情况下,气体供应被切断. 对于恒星质量低于10~11个太阳质量的星系,这个过程需要大约40亿年的时间.
科学领域:
- 天文学和天体物理学
- 银河系的进化 银河系的进化
- 恒星天体物理学 恒星天体物理学
背景情况:
- 星系被分为恒星形成 (气体丰富) 或静止 (气体贫乏) 的星系.
- 从恒星形成到静止状态的过渡的确切机制仍然是天体物理学中的一个关键问题.
- 拟议的火机制包括快速的气体去除 (外流/剥离) 和逐渐的气体供应饥饿 (窒息).
研究的目的:
- 调查负责灭局部星系恒星形成的主导机制.
- 为了确定与星系火相关的时间尺度.
- 分析恒星金属性和年龄在理解星系转变中的作用.
主要方法:
- 从26,000个银河系的光谱中分析恒星金属性.
- 静止和恒星形成星系之间的恒星年龄的比较.
- 专注于恒星质量小于10~11太阳质量的星系.
主要成果:
- 恒星金属性分析强烈表明杀是主要的火机制.
- 通过窒息火的典型时间表大约是40亿年.
- 在静止星系中观察到的年龄差异证实了40亿年的灭时间表.
结论:
- 窒息被确定为低质量局部星系中恒星形成火的主要驱动因素.
- 该研究为这种火过程提供了可靠的时间表.
- 这些发现支持逐渐切断气体供应作为银河系转变的关键.
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