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Investigating the properties of AGN feedback in hot atmospheres triggered by cooling-induced gravitational collapse

Citation

Pope, ECD and Mendel, TJ and Shabala, SS, Investigating the properties of AGN feedback in hot atmospheres triggered by cooling-induced gravitational collapse, Monthly Notices of the Royal Astronomical Society, 419, (1) pp. 50-56. ISSN 1365-2966 (2012) [Refereed Article]


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The definitive published version is available online at: http://www3.interscience.wiley.com/

DOI: doi:10.1111/j.1365-2966.2011.19669.x

Abstract

Radiative cooling may plausibly cause hot gas in the centre of a massive galaxy, or galaxy cluster, to become gravitationally unstable. The subsequent collapse of this gas on a dynamical timescale can provide an abundant source of fuel for AGN heating and star formation. Thus, this mechanism provides a way to link the AGN accretion rate to the global properties of an ambient cooling flow, but without the implicit assumption that the accreted material must have flowed onto the black hole from 10s of kiloparsecs away. It is shown that a fuelling mechanism of this sort naturally leads to a close balance between AGN heating and the radiative cooling rate of the hot, X-ray emitting halo. Furthermore, AGN powered by cooling-induced gravitational instability would exhibit characteristic duty cycles (δ) which are redolent of recent observational findings: δ ∝ LX3*, where LX is the X-ray luminosity of the hot atmosphere, and σ* is the central stellar velocity dispersion of the host galaxy. Combining this result with well-known scaling relations, we deduce a duty cycle for radio AGN in elliptical galaxies that is approximately ∝ M1.5BH, where MBH is the central black hole mass. Outburst durations and Eddington ratios are also given. Based on the results of this study, we conclude that gravitational instability could provide an important mechanism for supplying fuel to AGN in massive galaxies and clusters, and warrants further investigation.

Item Details

Item Type:Refereed Article
Keywords:hydrodynamics, instabilities, galaxies, active, galaxies, clusters, intracluster medium, elliptical and lenticular, cD
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Astronomical and Space Sciences not elsewhere classified
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Shabala, SS (Dr Stas Shabala)
ID Code:72561
Year Published:2012
Web of Science® Times Cited:8
Deposited By:Mathematics and Physics
Deposited On:2011-08-29
Last Modified:2017-11-03
Downloads:0

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