Feedback from radio-loud AGN

被引：29
|
作者：
Best, P. N. [1 ]
机构：
[1] Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
来源：
NEW ASTRONOMY REVIEWS | 2007年 / 51卷 / 1-2期
关键词：
galaxies : active; galaxies : evolution; accretion; radio continuum : galaxies; cooling flows;
D O I：
10.1016/j.newar.2006.11.014
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The evidence for direct interactions between radio-loud active galactic nuclei (AGN) and their surrounding gas is reviewed. New results from the Sloan Digital Sky Survey provide insightful information on the origin of radio-loud AGN activity, and allow study of the energetic influence of the radio-loud AGN on their surroundings, and the consequences of this for the accretion of gas onto elliptical galaxies. These results show that recurrent radio-loud AGN activity may provide a self-regulating feedback mechanism capable of controlling the rate of growth of galaxies. Finally, the effect of radio-loud AGN activity on gas at the scales of galaxy clusters is discussed. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码：168 / 173
页数：6
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