articleAnnual Review of Astronomy and AstrophysicsJun 27, 2014GREEN OA

The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe

TMTimothy M. HeckmanPNPhilip N. Best

Johns Hopkins University · Royal Observatory

Indexed inarxivcrossref

Abstract

We summarize what large surveys of the contemporary Universe have taught us about the physics and phenomenology of the processes that link the formation and evolution of galaxies with their central supermassive black holes. We present a picture in which the population of active galactic nuclei (AGNs) can be divided into two distinct populations. The radiative-mode AGNs are associated with black holes (BHs) that produce radiant energy powered by accretion at rates in excess of ∼1% of the Eddington limit. They are primarily associated with less massive BHs growing in high-density pseudobulges at a rate sufficient to produce the total mass budget in these BHs in ∼10 Gyr. The circumnuclear environment contains…

Citation impact

1,215
total citations
FWCI
42.48
Percentile
100%
References
438
Citations per year

Authors

2
  • TM
    Timothy M. HeckmanCorresponding

    Johns Hopkins University

  • PN
    Philip N. Best

    Royal Observatory

Topics & keywords

Keywords
  • Supermassive black hole
  • Active galactic nucleus
  • Bulge
  • Star formation
  • Galaxy
  • Accretion (finance)
  • Population
No related works found for this paper.