The First Galaxies

被引:373
作者
Bromm, Volker [1 ,2 ]
Yoshida, Naoki [3 ]
机构
[1] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA
[2] Univ Texas Austin, Texas Cosmol Ctr, Austin, TX 78712 USA
[3] Univ Tokyo, Inst Phys & Math Universe, Chiba 2778583, Japan
来源
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 49 | 2011年 / 49卷
基金
美国国家科学基金会;
关键词
cosmology; galaxy formation; intergalactic medium; Population III; star formation; SUPERMASSIVE BLACK-HOLES; POPULATION-III STARS; LY-ALPHA EMITTERS; INITIAL MASS FUNCTION; METAL-POOR STARS; RESONANCE-LINE RADIATION; ULTRA-FAINT DWARFS; DARK-MATTER HALOES; INTERGALACTIC C-IV; TO; GALAXIES;
D O I
10.1146/annurev-astro-081710-102608
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review our current understanding of how the first galaxies formed at the end of the cosmic dark ages a few 100 million years after the Big Bang. Modern large telescopes discovered galaxies at redshifts greater than seven, whereas theoretical studies have just reached the degree of sophistication necessary to make meaningful predictions. A crucial ingredient is the feedback exerted by the first generation of stars, through UV radiation, supernova blast waves, and chemical enrichment. The key goal is to derive the signature of the first galaxies to be observed with upcoming or planned next-generation facilities, such as the James Webb Space Telescope or Atacama Large Millimeter Array. From the observational side, ongoing deep-field searches for very high-redshift galaxies begin to provide us with empirical constraints on the nature of the first galaxies.
引用
收藏
页码:373 / 407
页数:35
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