Towards an understanding of the evolution of the scaling relations for supermassive black holes

The growth of the supermassive black holes (BHs) that reside at the centres of most galaxies is intertwined with the physical processes that drive the formation of the galaxies themselves. The evolution of the relations between the mass of the BH, m BH, and the properties of its host therefore repre...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2011-05, Vol.413 (2), p.1158-1164
Main Authors: Booth, C. M., Schaye, Joop
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Black holes
cosmology: theory
Dark matter
Earth, ocean, space
Exact sciences and technology
galaxies: active
galaxies: evolution
methods: numerical
quasars: general
Star & galaxy formation
Stars & galaxies
Thermodynamics
Online Access:Get full text
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