On the evolution of the black hole: spheroid mass ratio
Open Access
- 13 April 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 368 (3) , 1395-1403
- https://doi.org/10.1111/j.1365-2966.2006.10228.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 76 references indexed in Scilit:
- Self-regulated black hole accretion, the M- relation and the growth of bulges in galaxiesMonthly Notices of the Royal Astronomical Society, 2005
- Optical Spectrophotometry of a Complete Sample of 3CR Lobe-dominated QuasarsThe Astronomical Journal, 2005
- Constraints from Galaxy-AGN Clustering on the Correlation between Galaxy and Black Hole Mass at Redshift 2 ≲ z ≲ 3The Astrophysical Journal, 2005
- Iron Emission in the z = 6.4 Quasar SDSS J114816.64+525150.3The Astrophysical Journal, 2003
- A submillimetre survey of the star formation history of radio galaxiesMonthly Notices of the Royal Astronomical Society, 2001
- The cluster environments of the z 1 3CR radio galaxiesMonthly Notices of the Royal Astronomical Society, 2000
- HST, radio and infrared observations of 28 3CR radio galaxies at redshift z ∼ 1 — I. The observationsMonthly Notices of the Royal Astronomical Society, 1997
- MG II absorption in a sample of 56 steep-spectrum quasarsThe Astrophysical Journal Supplement Series, 1994
- Is every quasar beamed?The Astrophysical Journal, 1989
- 3C 216 - A new type of superluminal quasarThe Astrophysical Journal, 1988