The Coevolution of Galaxies and Supermassive Black Holes: A Local Perspective

被引：16
|
作者：
Heckman, Timothy M. [1 ]
Kauffmann, Guinevere [2 ]
机构：
[1] Johns Hopkins Univ, Ctr Astrophys Sci, Dept Phys & Astron, Baltimore, MD 21218 USA
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源：
SCIENCE | 2011年 / 333卷 / 6039期
关键词：
ACTIVE GALACTIC NUCLEI; DIGITAL SKY SURVEY; STAR-FORMATION; ELLIPTIC GALAXIES; BULGE MASS; EVOLUTION; LUMINOSITY; GROWTH; MODEL; FEEDBACK;
D O I：
10.1126/science.1200504
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
One of the most fascinating discoveries in the past decade was that galaxies typically contain a centrally located black hole with a mass that is millions or even billions of times that of the Sun. There is now compelling evidence that we cannot understand how galaxies formed and evolved without understanding the life cycles of these supermassive black holes (and vice versa). We summarize the current understanding of this coevolution of galaxies and supermassive black holes (based largely on observations of the local, present-day universe) and describe prospects for the future.
引用
收藏
页码：182 / 185
页数：4
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