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The Co-Evolution of Supermassive Black Holes and Galaxies: Observational Constraints

Published online by Cambridge University Press:  17 July 2013

Xian Zhong Zheng
Xian Zhong Zheng*
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, 2 West-Beijing Road, Nanjing 210008, P. R. China email: xzzheng@pmo.ac.cn
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Abstract

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The connection between the growth of supermassive black holes (SMBHs) and the assembly of their host galaxies is termed ‘co-evolution’. Understanding co-evolution is one of the most fundamental issues in modern astrophysics. In this contribution, we review recent progress in addressing how the growth of SMBHs is linked to the properties of their host galaxies in the context of galaxy evolution, from the observational point of view. Although a coherent picture has not yet emerged, multiple pathways of co-evolution appear to be favored with a probable dependence on AGN luminosity and redshift.

Keywords

galaxies: generalgalaxies: evolutiongalaxies: nucleiquasars: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 109 - 116
Copyright
Copyright © International Astronomical Union 2013 

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