The cosmological history of accretion onto dark halos and supermassive black holes

2006/08/10 by L. Miller, W. J. Percival, Will J. Percival +3 · 2 citations
Physics and Astronomy · #Accretion (finance) #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gamma-ray burst progenitors #Halo #Intermediate-mass black hole #Physics #Supermassive black hole #astro-ph

paper · pdf · doi:10.1051/0004-6361:20064945

14 pages. Accepted for publication in Astronomy and Astrophysics

arxiv created 2006/08/10 · openalex publication_date 2006/08/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. We investigate the cosmological growth of dark halos and follow the consequences of coeval growth for the accretion history of associated supermassive black holes.

Citations

• Black hole winds
• The Demography of Massive Dark Objects in Galaxy Centers
• Cosmological evolution and hierarchical galaxy formation
• Black Holes in Galaxy Mergers: Evolution of Quasars
• Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the Black Hole Mass–Velocity Dispersion Relationship for Active Galactic Nuclei
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion
• A 3 × 10[TSUP]9[/TSUP] [ITAL]M[/ITAL][TINF]⊙[/TINF] Black Hole in the Quasar SDSS J1148+5251 at [CLC][ITAL]z[/ITAL][/CLC] = 6.41

Cited by

• THE PSEUDO-EVOLUTION OF HALO MASS
• Jet-regulated cooling catastrophe