Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Galaxy mergers in eagle do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN.

Patton, David R. and Johansson, Peter H. and Ellison, Sara L. and Alexander, David M. and Rosario, David J. and Harrison, Chris M. and McAlpine, Stuart (2020) 'Galaxy mergers in eagle do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN.', Monthly notices of the Royal Astronomical Society. .

Abstract

We investigate the connection between galaxy–galaxy mergers and enhanced black hole (BH) growth using the cosmological hydrodynamical eagle simulation. We do this via three methods of analysis, investigating: the merger fraction of AGN, the AGN fraction of merging systems and the AGN fraction of galaxies with close companions. In each case, we find an increased abundance of AGN within merging systems relative to control samples of inactive or isolated galaxies (by up to a factor of ≈ 3 depending on the analysis method used), confirming that mergers are enhancing BH accretion rates for at least a subset of the galaxy population. The greatest excess of AGN triggered via a merger are found in lower mass (푀∗ ∼ 1010 M) gas rich ( 푓gas > 0.2) central galaxies with lower mass BHs (푀BH ∼ 107 M) at lower redshifts (푧 < 1). We find no enhancement of AGN triggered via mergers in more massive galaxies (푀∗ & 1011 M). The enhancement of AGN is not uniform throughout the phases of a merger, and instead peaks within the early remnants of merging systems (typically lagging ≈ 300 Myr post-coalescence of the two galaxies at 푧 = 0.5). We argue that neither major (푀∗,1/푀∗,2 ≥ 1 4 ) nor minor mergers ( 1 10 < 푀∗,1/푀∗,2 < 1 4 ) are statistically relevant for enhancing BH masses globally. Whilst at all redshifts the galaxies experiencing a merger have accretion rates that are on average 2–3 times that of isolated galaxies, the majority of mass that is accreted onto BHs occurs outside the periods of a merger. We compute that on average no more than 15% of a BHs final day mass comes from the enhanced accretion rates triggered via a merger.

Item Type:Article
Full text:(AM) Accepted Manuscript
Download PDF
(4589Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnras/staa1123
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:No date available
Date deposited:28 April 2020
Date of first online publication:2020
Date first made open access:28 April 2020

Save or Share this output

Export:
Export
Look up in GoogleScholar