Q Ni
Does black hole growth depend fundamentally on host-galaxy compactness?
Ni, Q; Yang, G; Brandt, WN; Alexander, DM; Chen, C-TJ; Luo, B; Vito, F; Xue, YQ
Authors
G Yang
WN Brandt
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
C-TJ Chen
B Luo
F Vito
YQ Xue
Abstract
Possible connections between central black hole (BH) growth and host-galaxy compactness have been found observationally, which may provide insight into BH–galaxy coevolution: compact galaxies might have large amounts of gas in their centres due to their high mass-to-size ratios, and simulations predict that high central gas density can boost BH accretion. However, it is not yet clear if BH growth is fundamentally related to the compactness of the host galaxy, due to observational degeneracies between compactness, stellar mass (M⋆) and star formation rate (SFR). To break these degeneracies, we carry out systematic partial-correlation studies to investigate the dependence of sample-averaged BH accretion rate (BHAR¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯) on the compactness of host galaxies, represented by the surface-mass density, Σe, or the projected central surface-mass density within 1 kpc, Σ1. We utilize 8842 galaxies with H < 24.5 in the five CANDELS fields at z = 0.5–3. We find that BHAR¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯ does not significantly depend on compactness when controlling for SFR or M⋆ among bulge-dominated galaxies and galaxies that are not dominated by bulges, respectively. However, when testing is confined to star-forming galaxies at z = 0.5–1.5, we find that the BHAR¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯–Σ1 relation is not simply a secondary manifestation of a primary BHAR¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯–M⋆ relation, which may indicate a link between BH growth and the gas density within the central 1 kpc of galaxies.
Citation
Ni, Q., Yang, G., Brandt, W., Alexander, D., Chen, C., Luo, B., …Xue, Y. (2019). Does black hole growth depend fundamentally on host-galaxy compactness?. Monthly Notices of the Royal Astronomical Society, 490(1), 1135-1155. https://doi.org/10.1093/mnras/stz2623
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 11, 2019 |
Online Publication Date | Sep 19, 2019 |
Publication Date | Nov 30, 2019 |
Deposit Date | Dec 6, 2019 |
Publicly Available Date | Dec 6, 2019 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 490 |
Issue | 1 |
Pages | 1135-1155 |
DOI | https://doi.org/10.1093/mnras/stz2623 |
Public URL | https://durham-repository.worktribe.com/output/1281696 |
Files
Published Journal Article
(9.8 Mb)
PDF
Copyright Statement
This article has been accepted for publication in the Monthly notices of the Royal Astronomical Society ©: 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
The high energy X-ray probe (HEX-P): bringing the cosmic X-ray background into focus
(2024)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.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