Modeling DM and ICM in simulated galaxy clusters

Details Modeling DM and ICM in simulated galaxy clusters Modeling DM and ICM in simulated galaxy clusters

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ogci.conf..309r&link_type=abstract

Outskirts of Galaxy Clusters: Intense Life in the Suburbs. Edited by Antonaldo Diaferio, IAU Colloquium #195, p.309-312

Physics

Scientific paper

Using the results of an extended set of high-resolution non-radiative
hydrodynamic simulations of galaxy clusters we obtain simple analytic
formulae for the dark matter and hot gas distribution, in the spherical
approximation.

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