Keele Research Repository
Explore the Repository
Tools
Larkin, AC and McLaughlin, DE (2016) Dark-matter haloes and the M-sigma relation for supermassive black holes. Monthly Notices of the Royal Astronomical Society, 462 (2). 1864 -1881. ISSN 1365-2966
Preview
larkin_2016_stw1749.pdf - Published Version
Download (771kB) | Preview
Official URL: http://dx.doi.org/10.1093/mnras/stw1749
Abstract
We develop models of two-component spherical galaxies to establish scaling relations linking the properties of spheroids at z = 0 (total stellar masses, effective radii Re and velocity dispersions within Re) to the properties of their dark-matter haloes at both z = 0 and higher redshifts. Our main motivation is the widely accepted idea that the accretion-driven growth of supermassive black holes (SMBHs) in protogalaxies is limited by quasar-mode feedback and gas blow-out.
Item Type: | Article |
---|---|
Additional Information: | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Uncontrolled Keywords: | galaxies, bulges, elliptical and lenticular, cD, fundamental, parameters, haloes, quasars, supermassive black holes |
Subjects: | Q Science > QB Astronomy > QB460 Astrophysics Q Science > QB Astronomy > QB799 Stars |
Divisions: | Faculty of Natural Sciences > School of Physical and Geographical Sciences |
Related URLs: | |
Depositing User: | Symplectic |
Date Deposited: | 03 Feb 2017 16:12 |
Last Modified: | 19 Sep 2017 14:03 |
URI: | https://eprints.keele.ac.uk/id/eprint/2865 |
Actions (login required)
Altmetric