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一个星系的红移z = 6.96的星系.
Masanori Iye1, Kazuaki Ota, Nobunari Kashikawa
1National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan. iye@optik.mtk.nao.ac.jp
Nature
|September 15, 2006
概括
早期的星系形成是由一个在红移z = 6.96的光谱识别的星系证实的,可以追溯到大爆炸后7.5亿年. 这一发现揭示了银河系组合在宇宙历史的早期非常活跃.
科学领域:
- 宇宙学的宇宙学是什么?
- 银河系的形成和进化
- 早期宇宙天体物理学 天体物理学
背景情况:
- 早期宇宙中星系形成的精确时间还不清楚.
- 宇宙微波背景研究表明,再电离发生在红移z=6和14之间.
- 以前对星系的光谱证据仅限于z < 6.6,尽管光度候选人在更高的红移.
研究的目的:
- 用光谱学方法证实存在非常高红移 (z > 7) 的星系.
- 研究早期宇宙中星系形成和恒星形成活动的开始.
- 为了确定z处的星系的数密度,大约是7.
主要方法:
- 在高红移的候选星系的光谱观测.
- 对银河系的光谱进行分析,以确定辐射线,特别是莱曼-alpha.
- 确定银河系的红移和估计其恒星形成率.
主要成果:
- 一个星系获得了z = 6.96的光谱红移,相当于大爆炸后的7.5亿年.
- 银河系的光谱表现出突出的莱曼-α辐射,表明活跃的恒星形成.
- 估计恒星形成速度大约是每年10个太阳质量.
结论:
- 当宇宙只有大约6%的当前年龄时,银河系的形成正在积极发生.
- 星系的数量密度在z约为7时明显低 (18-36%),而不是z=6.6.
- 这一发现推动了确认早期星系形成的观测前沿.
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