EROs and faint red galaxies

被引：58

作者：

McCarthy, PJ ^{[1
]}

机构：

[1] Carnegie Inst Washington Observ, Pasadena, CA 91101 USA

来源：

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 2004年 / 42卷

关键词：

galaxy evolution; galaxy formation; infrared surveys; starburst galaxies;

D O I：

10.1146/annurev.astro.42.053102.134032

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This chapter reviews the properties of faint IR-selected field galaxies and the extremely red color-selected populations in particular. These populations are a mix of passively evolving stellar systems and heavily obscured star-forming galaxies. The star-forming component appears to constitute 20-50% of the population depending on the magnitude and color cuts employed. The remaining objects are a mix of passively evolving ellipticals and early-type disk galaxies. The passively evolving red galaxies are strongly clustered in space and are likely the high-mass high-luminosity end of the elliptical galaxy progenitor population at redshifts between one and two. These galaxies have masses and space densities that appear to be in conflict with late-forming hierarchical galaxy-formation models. The red galaxies appear to be a population that is distinct from the moderately star-forming Lyman-Break galaxies but may be related to the starburst population at z > 2 seen in deep submillimeter surveys.

引用

页码：477 / 515

页数：47

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