银河系在宇宙历史上第一个十亿年的巨大光环增长
D P Marrone1, J S Spilker1, C C Hayward2,3
1Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721, USA.
Nature
|December 7, 2017
概括
天文学家发现一对大质量,合并的星系在红移6.9,大爆炸后不到8亿年. 这一发现揭示了罕见的早期宇宙结构,
科学领域:
- 宇宙学
- 星系的形成和演变
- 早期宇宙的天体物理学
背景情况:
- 宇宙结构形成模型预测高密度区域的早期星系前体.
- 由于检测灵敏度和测量宽度的要求,观察这些早期的大型结构具有挑战性.
- 很少有这样的物体被探测到, 这凸显了早期大质量星系的罕见性.
研究的目的:
- 报告一个罕见的,远红外发光物体的发现和特征.
- 在早期宇宙中研究极大质量的恒星形成星系的特性.
- 了解早期大质量星系的形成机制和环境影响.
主要方法:
- 使用广场测量来初步检测遥远的发光物体.
- 使用高分辨率成像来解析检测到的物体的结构.
- 分析了光谱数据以确定红移,恒星形成率和气体/尘埃含量.
主要成果:
- 发现了一对合并的极大质量恒星形成星系,红移6.9 (约. 大爆炸后的8亿年).
- 这个较大的星系的恒星形成速度为每年2900个太阳质量,有270亿个太阳质量的气体和25亿个太阳质量的尘埃.
- 伴星系有35亿个太阳质量的恒星,恒星形成速度为540个太阳质量/年,气体和尘埃明显减少.
结论:
- 观测到的星系表明存在一个超过1000亿太阳质量的暗物质光环,
- 在更大的星系中快速形成的恒星很可能是由其合并的伴侣引发的.
- 这些发现为早期宇宙中最庞大的宇宙结构的组合提供了关键的见解.
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