Galactic winds

被引：1247

作者：

Veilleux, S ^{[1
]}

Cecil, G

Bland-Hawthorn, J

机构：

[1] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[2] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA

[3] Anglo Australian Observ, Epping, NSW 2121, Australia

来源：

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 2005年 / 43卷

关键词：

evolution; halos; intergalactic medium; kinematics and dynamics; nuclei;

D O I：

10.1146/annurev.astro.43.072103.150610

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Galactic winds are the primary mechanism by which energy and metals are recycled in galaxies and are deposited into the intergalactic medium. New observations are revealing the ubiquity of this process, particularly at high redshift. We describe the physics behind these winds, discuss the observational evidence for them in nearby star-forming and active galaxies and in the high-redshift universe, and consider the implications of energetic winds for the formation and evolution of galaxies and the intergalactic medium. To inspire future research, we conclude with a set of observational and theoretical challenges.

引用

页码：769 / 826

页数：58

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