Can simulations reproduce the observed temperature-mass relation for clusters of galaxies?

Thomas, P.A., Muanwong, O., Kay, S.T. and Liddle, A.R. (2002) Can simulations reproduce the observed temperature-mass relation for clusters of galaxies? Monthly Notices of the Royal Astronomical Society, 330 (2). L48-L52. ISSN 0035-8711

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Abstract

It has become increasingly apparent that traditional hydrodynamical simulations of galaxy clusters are unable to reproduce the observed properties of galaxy clusters, in particular overpredicting the mass corresponding to a given cluster temperature.

Item Type: Article
Keywords: hydrodynamics - methods: N-body simulations - galaxies: clusters: general - X-rays: galaxies: clusters.
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Subjects: Q Science > QB Astronomy
Depositing User: Sarah Pelling
Date Deposited: 03 Oct 2008
Last Modified: 07 Mar 2017 08:34
URI: http://sro.sussex.ac.uk/id/eprint/1895
Google Scholar:45 Citations

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