What drives the growth of black holes?

被引：498

作者：

Alexander, D. M. ^{[1
]}

Hickox, R. C. ^{[1
,2
]}

机构：

[1] Univ Durham, Dept Phys, Durham DH1 3LE, England

[2] Dartmouth Coll, Dept Phys & Astron, Wilder Lab 6127, Hanover, NH 03755 USA

来源：

NEW ASTRONOMY REVIEWS | 2012年 / 56卷 / 04期

基金：

英国科学技术设施理事会;

关键词：

ACTIVE GALACTIC NUCLEI; DIGITAL-SKY-SURVEY; DEEP-FIELD-SOUTH; DARK-MATTER HALOES; ULTRALUMINOUS INFRARED GALAXIES; STAR-FORMING GALAXIES; DWARF SEYFERT NUCLEI; SGR-A-ASTERISK; SPECTRAL ENERGY-DISTRIBUTIONS; EXTRAGALACTIC RADIO-SOURCES;

D O I：

10.1016/j.newar.2011.11.003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of massive galaxies in the local Universe. Recent years have seen remarkable advances in our understanding of how these BHs form and grow over cosmic time, during which they are revealed as Active Galactic Nuclei (AGN). However, despite decades of research, we still lack a coherent picture of the physical drivers of BH growth, the connection between the growth of BHs and their host galaxies, the role of large-scale environment on the fueling of BHs, and the impact of BH-driven outflows on the growth of galaxies. In this paper we review our progress in addressing these key issues, motivated by the science presented at the "What drives the growth of black holes?" workshop held at Durham on 26-29th July 2010, and discuss how these questions may be tackled with current and future facilities. (C) 2011 Elsevier B.V. All rights reserved.

引用

页码：93 / 121

页数：29

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