Self-regulated black hole accretion, the M- relation and the growth of bulges in galaxies
Open Access
- 21 August 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 361 (4) , 1387-1392
- https://doi.org/10.1111/j.1365-2966.2005.09249.x
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This publication has 28 references indexed in Scilit:
- Energy input from quasars regulates the growth and activity of black holes and their host galaxiesNature, 2005
- Two-dimensional adiabatic flows on to a black hole – I. Fluid accretionMonthly Notices of the Royal Astronomical Society, 2004
- Formation of Supermassive Black Holes in Galactic Bulges: A Rotating Collapse Model Consistent with theMBH‐σ RelationThe Astrophysical Journal, 2003
- On the detectability of distant Compton-thick obscured quasarsMonthly Notices of the Royal Astronomical Society, 2002
- Profiles of dark haloes: evolution, scatter and environmentMonthly Notices of the Royal Astronomical Society, 2001
- The obscured growth of massive black holesMonthly Notices of the Royal Astronomical Society, 1999
- On the fate of gas accreting at a low rate on to a black holeMonthly Notices of the Royal Astronomical Society, 1999
- Statistical Properties of X‐Ray Clusters: Analytic and Numerical ComparisonsThe Astrophysical Journal, 1998
- Can a spherically accreting black hole radiate very near the Eddington limitMonthly Notices of the Royal Astronomical Society, 1979
- Velocity dispersions and mass-to-light ratios for elliptical galaxiesThe Astrophysical Journal, 1976