REVISITING THE SCALING RELATIONS OF BLACK HOLE MASSES AND HOST GALAXY PROPERTIES
- 5 February 2013
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 764 (2)
- https://doi.org/10.1088/0004-637x/764/2/184
Abstract
No abstract availableOther Versions
This publication has 100 references indexed in Scilit:
- An over-massive black hole in the compact lenticular galaxy NGC 1277Nature, 2012
- Radially extended kinematics and stellar populations of the massive ellipticals NGC 1600, NGC 4125, and NGC 7619Astronomy & Astrophysics, 2010
- Black hole growth in hierarchical galaxy formationMonthly Notices of the Royal Astronomical Society, 2007
- The supermassive black hole in NGC 4486a detected with SINFONI at the Very Large TelescopeMonthly Notices of the Royal Astronomical Society, 2007
- The black hole mass - spheroid luminosity relationMonthly Notices of the Royal Astronomical Society, 2007
- The Luminosities, Sizes, and Velocity Dispersions of Brightest Cluster Galaxies: Implications for Formation HistoryThe Astronomical Journal, 2007
- A Log‐Quadratic Relation for Predicting Supermassive Black Hole Masses from the Host Bulge Sersic IndexThe Astrophysical Journal, 2007
- Red mergers and the assembly of massive elliptical galaxies: the fundamental plane and its projectionsMonthly Notices of the Royal Astronomical Society, 2006
- On the Correlations of Massive Black Holes with Their Host GalaxiesThe Astrophysical Journal, 2006
- Kinematics of 10 Early‐Type Galaxies fromHubble Space Telescopeand Ground‐based SpectroscopyThe Astrophysical Journal, 2003