Interaction of Supermassive Black Holes with their Stellar and Dark Matter Environments
arXiv:astro-ph/0409290 · doi:10.1007/11403913_44
Abstract
A review of recent theoretical work on the interactions of supermassive single and binary black holes with their nuclear environments, highlighting ways in which the observed structure of nuclei can be used to constrain the formation history of black holes.
15 pages, to appear in "Growing Black Holes: Accretion in Cosmological Context"