早期宇宙中的一个动态冷盘星系
F Rizzo1, S Vegetti2, D Powell2
1Max-Planck Institute for Astrophysics, Garching, Germany. frizzo@mpa-garching.mpg.de.
Nature
|August 14, 2020
概括
早期的星系被认为是混乱的. 然而,我们发现一个动态冷的旋转圆盘星系, 红移z=4.2,
科学领域:
- 宇宙进化
- 星系的形成和动态
背景情况:
- 早期的宇宙条件 (极端的天体物理过程,融合,超新星) 预测形成动态热,混乱和不稳定的年轻星系.
- 目前的模型表明,由于这些极端条件,早期和本地宇宙星系之间存在显著差异.
研究的目的:
- 在早期宇宙中研究星系的动态特性.
- 为了确定年轻星系是否会有秩序的旋转,并且有动态冷,类似于局部星系.
主要方法:
- 使用高空间分辨率的干扰度成像 (约. 60个帕塞克) 来研究星系SPT-S J041839-4751.
- 分析了旋转与随机运动的比率, 并推导出银河系的旋转曲线.
- 通过引力透镜观察遥远的星系.
主要成果:
- 在一个星系中发现了一个动态冷的,高度形成恒星的旋转盘,红移z=4.2 (宇宙年龄约14亿年).
- 测量了旋转和随机运动的比率 (9.7 ± 0.4),明显高于这个时代的模型预测.
- 一个旋转曲线的形状与附近的大型螺旋星系一致.
结论:
- 至少一些早期宇宙中的星系是动态冷的,有秩序的,类似于局部螺旋星系.
- 这些发现挑战了所有年轻星系都受到极端早期宇宙过程的强烈影响的观点.
- 这表明银河系的进化途径甚至可以在新生的宇宙中导致动态冷盘.
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