一个120亿年前的星体爆发的引力不稳定的气体盘
K Tadaki1, D Iono2,3, M S Yun4
1National Astronomical Observatory of Japan, Tokyo, Japan. tadaki.ken@nao.ac.jp.
Nature
|August 31, 2018
概括
早期宇宙中的星系在紧的尘土核心中迅速形成恒星. 这些星爆核在引力上不稳定,
科学领域:
- 天文学与天体物理学
- 宇宙进化
- 星系的形成
背景情况:
- 早期宇宙中的亚毫米星系的恒星形成率比银河系高1000倍.
- 这种恒星形成的很大一部分集中在紧的中央千帕塞克区域.
- 由于需要高角度分辨率,了解这些核心的物理和动力特性是具有挑战性的.
研究的目的:
- 为了研究一个微米亮度星系的模糊核心中分子气体的空间和动态结构,红移z=4.3.
- 为了确定这些紧的星爆核心中的气体盘是否在旋转上受支持并且在引力上不稳定.
- 估计这些早期宇宙星系中恒星形成的气体消耗时间表.
主要方法:
- 在z=4.3的未透镜亚毫米亮星系中观察到气体和尘埃.
- 实现了550帕塞克的线性分辨率, 实现了星系核心的详细探测.
- 分析分子气体特性,包括每单位面积的质量和动力学 (旋转速度与速度分散).
主要成果:
- 在重度尘埃覆盖的核心中解决了分子气体的空间和动力结构.
- 证明气体盘是块状和旋转支持的,旋转速度超过速度分散.
- 分析表明星爆盘在引力上是不稳定的, 自重力主导着旋转和反压力.
结论:
- 在星爆盘中观察到的引力不稳定性表明恒星形成的气体消耗很快.
- 预计分子气体的消耗时间大约为1亿年.
- 这种快速消耗的时间尺度与在星际爆炸星系的合并中观察到的时间尺度相似.
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