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在早期宇宙中占主导地位的光学不可见的巨大星系
T Wang1,2,3, C Schreiber4,5,6, D Elbaz4
1Institute of Astronomy, Graduate School of Science, The University of Tokyo, Tokyo, Japan. twang.nju@gmail.com.
Nature
|August 9, 2019
概括
在早期的宇宙中, 巨大的尘土星系曾经被忽视. 这些新发现的星系显著增加了早期宇宙恒星形成的估计,并挑战了当前的星系形成模型.
科学领域:
- 宇宙的演化
- 星系的形成和演变
- 早期宇宙的天体物理学
背景情况:
- 在红移z > 3时的宇宙恒星形成历史主要使用紫外线选择的星系进行研究.
- 紫外线测量不足以代表大质量,富有尘埃和/或老恒星群的星系.
- 之前的研究发现极端星系爆发, 而不是大规模早期星系.
研究的目的:
- 在早期宇宙中研究大量星系和恒星形成率密度 (z > 3).
- 在紫外线和近红外线中隐藏的巨大星系.
- 描述这个以前错过的群体的特性和宇宙贡献.
主要方法:
- 在870微米处进行亚毫米观测以检测尘埃遮蔽的星系.
- 分析深紫外线到近红外光谱区域以识别未遮蔽的星系.
- 探测到的星系的空间密度和恒星形成率的估计.
主要成果:
- 探测到39个巨大的恒星形成星系在z>3,此前在紫外线到近红外测量中未见过.
- 这些星系的空间密度比极端星体爆发高两倍.
- 它们的恒星形成速率每年约为200太阳质量,对早期宇宙的恒星形成速率密度做出了重大贡献.
结论:
- 大规模的尘土星系是早期宇宙中重要且被低估的组成部分.
- 它们的丰富性挑战了目前的大规模星系形成的模型.
- 这些星系很可能是当今巨型星系的祖先.
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