The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
Johns Hopkins University · Royal Observatory
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
- FWCI
- 42.48
- Percentile
- 100%
- References
- 438
Authors
2- TMTimothy M. HeckmanCorresponding
Johns Hopkins University
- PNPhilip N. Best
Royal Observatory
Topics & keywords
- Supermassive black hole
- Active galactic nucleus
- Bulge
- Star formation
- Galaxy
- Accretion (finance)
- Population