We summarize our recent results on the evolution of super-massive black holes in the cores of galaxies. Our models are based on the viscous, Eddington-limited evolution of self-gravitating accretion disks. We find that, within this framework, one can explain the growth time scales and the luminosities of individual objects as well as the variation of these quantities for AGN with different black hole masses.
|Original language||English (US)|
|Journal||Journal of Physics: Conference Series|
|State||Published - Jan 1 2012|
|Event||Astronomy at High Angular Resolution 2011: The Central Kiloparsec in Galactic Nuclei, AHAR 2011 - Bad Honnef, Germany|
Duration: Aug 29 2011 → Sep 2 2011
ASJC Scopus subject areas
- Physics and Astronomy(all)