Close, JL, Pittard, JM, Hartquist, TW et al. (1 more author) (2013) Ram pressure stripping of the hot gaseous haloes of galaxies using the k - ε sub-grid turbulence model. Monthly Notices of the Royal Astronomical Society, 436 (4). 3021 - 3030. ISSN 0035-8711
Abstract
We perform three-dimensional hydrodynamic simulations of the ram pressure stripping of the hot extended gaseous halo of a massive galaxy using the k - ε sub-grid turbulence model at Mach numbers 0.9, 1.1 and 1.9. The k - ε model is used to simulate high Reynolds number flows by increasing the transport coefficients in regions of high turbulence. We find that the initial, instantaneous stripping is the same whether or not the k - ε model is implemented and is in agreement with the results of other studies. However the use of the k - ε model leads to five times less gas remaining after stripping by a supersonic flow has proceeded for 10 Gyr, which is more consistent with what simple analytic calculations indicate. Hence the continual Kelvin-Helmholtz stripping plays a significant role in the ram pressure stripping of the haloes of massive galaxies. To properly account for this, simulations of galaxy clusters will require the use of sub-grid turbulence model.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2013, The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Keywords: | Clusters; evolution - galaxies; general- galaxies; haloes; hydrodynamics - methods; numerical - galaxies |
Dates: |
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Institution: | The University of Leeds |
Academic Units: | The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds) |
Depositing User: | Symplectic Publications |
Date Deposited: | 22 Jan 2015 12:05 |
Last Modified: | 18 Jan 2018 03:11 |
Published Version: | http://dx.doi.org/10.1093/mnras/stt1788 |
Status: | Published |
Publisher: | Oxford University Press |
Identification Number: | 10.1093/mnras/stt1788 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:82594 |