一个巨大的静止星系在红移4.658
Adam C Carnall1, Ross J McLure2, James S Dunlop2
1Institute for Astronomy, School of Physics & Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK. adam.carnall@ed.ac.uk.
Nature
|May 22, 2023
概括
天文学家发现了一个巨大的静止星系GS-9209, 这个星系在灭之前迅速形成恒星, 挑战星系形成模型.
科学领域:
- 太空历史
- 星系的形成和演变
- 早期宇宙的天体物理学
背景情况:
- 早期星系的快速聚集挑战了当前的星系形成物理学.
- 詹姆斯·韦伯太空望远镜 (JWST) 证实了许多早期的星系,加剧了这个难题.
- 巨大的静止星系迅速形成,然后停止恒星形成, 在宇宙历史的早期被观察到令人惊.
研究的目的:
- 通过光谱检测证实在宇宙早期存在巨大的静止星系.
- 研究这些极端早期星系的特性和形成历史.
- 了解星系形成模型的含义.
主要方法:
- 使用JWST近红外光谱仪 (NIRSpec) 进行光谱观测.
- 分析了光谱数据以确认红移和推断星系属性.
- 确定恒星质量和恒星形成历史.
主要成果:
- 一个巨大的静止星系的光谱确认,GS-9209,红移z=4.658 (大爆炸后的125亿年).
- 推断的恒星质量为3.8 ± 0.2 × 10^10 M.
- 确定GS-9209在宇宙大约800亿年时迅速形成恒星.
结论:
- 在宇宙的早期形成的一个巨大的静止星系.
- 这一发现为快速的星系组合和灭提供了重要的观测证据.
- 这个星系是早期高红移物体与大质量局部星系之间的潜在联系.
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