Dynamics of galaxy cores and supermassive black holes
arXiv:astro-ph/0605070 · doi:10.1088/0034-4885/69/9/R01
Abstract
Recent work on the dynamical evolution of galactic nuclei containing supermassive black holes is reviewed. Topics include galaxy structural properties; collisionless and collisional equilibria; loss-cone dynamics; and dynamics of binary and multiple supermassive black holes.
75 pages, 28 figures. To appear in Reports on Progress in Physics
References in corpus (6)
- The ACS Virgo Cluster Survey. VIII. The Nuclei of Early-Type Galaxies
- A Compact Supermassive Binary Black Hole System
- From Supermassive Black Holes to Dwarf Elliptical Nuclei: a Mass Continuum
- X-ray Detection of the Proto Supermassive Binary Black Hole at the Centre of Abell 400
- The Lyman-alpha glow of gas falling into the dark matter halo of a z=3 galaxy
- The Nuclear Orbital Distribution in Galaxies as Fossil Record of Black Hole Formation from Integral-Field Spectroscopy
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- Interaction of massive black hole binaries with their stellar environment: III. Scattering of bound stars
- The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
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- The Formation of Intermediate Mass Black Holes in Galactic Nuclei
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- The role of thermal evaporation in galaxy formation
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- The Evolutionary History of Galactic Bulges: Photometric and Spectroscopic Studies of Distant Spheroids in the GOODS Fields
- Aligning Retrograde Nuclear Cluster Orbits with an Active Galactic Nucleus Accretion Disc
- On the relation between the mass of Compact Massive Objects and their host galaxies
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- On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
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- Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
- SZ effects from annihilating dark matter in the Milky Way: smooth halo, subhalos and intermediate-mass-black-holes
- Holes within galaxies: the egg or the hen?
- The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
- Physically motivated fit to mass surface density profiles observed in galaxies
- SDSS J153231.80+420342.7: a triple black hole candidate with a close binary black hole