Nature versus Nurture: The curved spine of the galaxy cluster X-ray luminosity – temperature relation

Hartley, W., Gazzola, L., Pearce, F.R., Kay, S.T. and Thomas, P.A. (2008) Nature versus Nurture: The curved spine of the galaxy cluster X-ray luminosity – temperature relation. Monthly Notices of the Royal Astronomical Society, 386 (4). pp. 2015-2021. ISSN 0035-8711

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Abstract

The physical processes that define the spine of the galaxy cluster X-ray luminosity-temperature (L-T) relation are investigated using a large hydrodynamical simulation of the universe.

Item Type: Article
Keywords: hydrodynamics - methods: numerical - cosmology: theory.
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 08:33
URI: http://sro.sussex.ac.uk/id/eprint/1924

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