STAR FORMATION QUENCHING IN GALAXIES

被引：0

作者：

Kimm, T. ^{[1
]}

Somerville, R. S. ^{[2
,3
]}

Yi, S. K. ^{[1
]}

van den Bosch, F. C. ^{[3
]}

Salim, S. ^{[4
]}

Fontonot, F. ^{[3
]}

Monaco, P. ^{[5
,6
]}

Mo, H. J. ^{[7
]}

Pasquali, A. ^{[3
]}

Rich, R. M. ^{[8
]}

Yang, X. ^{[9
]}

机构：

[1] Yonsei Univ, Dept Astron, Seoul 120749, South Korea

[2] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[3] Max Planck Inst Astron, D-69117 Heidelberg, Germany

[4] Natl Opt Astron Observ, Tucson, AZ 85719 USA

[5] Univ Trieste, Dipartimento Astron, I-34143 Trieste, Italy

[6] INAF Osservatorio Astron, I-34143 Trieste, Italy

[7] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[8] Univ Calif San Diego, Dept Phys & Astron, San Diego, CA USA

[9] Shanghai Astron Observ, Shanghai, Peoples R China

来源：

ROLE OF THE DISK-HALO INTERACTION IN GALAXY EVOLUTION: OUTFLOWS VS INFALL? | 2012年 / 56卷

关键词：

D O I：

10.1051/eas/1256025

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate the correlation of star formation quenching with internal galaxy properties and environment by comparing observation and theoretical models. We first classify galaxies as the most massive "central" or "satellite" in each halo in order to investigate the environmental effect. For observed central galaxies, we are unable to determine whether star formation quenching is primarily connected with halo mass or stellar mass, because these two quantities are strongly correlated. For satellite galaxies, a nearly equal dependence on halo mass and stellar mass is seen. We find that theoretical models with AGN feedback reproduce the dependence on colours and specific star formation rates for central galaxies reasonably. However, the same models seriously fail to reproduce the star formation rates of satellite galaxies by over-quenching star formation via strong strangulation: satellite over-quenching problem.

引用

页码：167 / +

页数：2

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