The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties

Kay, S.T., da Silva, A.C., Aghanim, N., Blanchard, A., Liddle, A.R., Puget, J.-L., Sadat, R. and Thomas, P.A. (2007) The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties. Monthly Notices of the Royal Astronomical Society, 377 (1). pp. 317-334. ISSN 0035-8711

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Abstract

We present results from a study of the X-ray cluster population that forms within the CLEF cosmological hydrodynamics simulation, a large N-body/SPH simulation of the Lambda cold dark matter cosmology with radiative cooling, star formation and feedback.

Item Type: Article
Keywords: hydrodynamics - methods: numerical - 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 08:35
URI: http://sro.sussex.ac.uk/id/eprint/1920
Google Scholar:57 Citations

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