larkin_2016_stw1749.pdf
(772 Kb)
PDF
Dark-matter haloes and the M-sigma relation for supermassive black holes
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.
Acceptance Date | Jul 17, 2016 |
---|---|
Publication Date | Oct 21, 2016 |
Publicly Available Date | Mar 28, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Pages | 1864 -1881 |
DOI | https://doi.org/10.1093/mnras/stw1749 |
Keywords | galaxies, bulges, elliptical and lenticular, cD, fundamental, parameters, haloes, quasars, supermassive black holes |
Publisher URL | http://dx.doi.org/10.1093/mnras/stw1749 |
Files
Downloadable Citations
About Keele Repository
Administrator e-mail: research.openaccess@keele.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search