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The effect of non--gravitational gas heating in...
Preprint

The effect of non--gravitational gas heating in groups and clusters of galaxies

Abstract

We present a set of gas-dynamical simulations of galaxy groups and clusters aimed at exploring the effect of non-gravitational heating. We use GASOLINE, a parallel Tree+SPH code, to simulate the formation of four cosmic halos with temperature 0.5

Authors

Borgani S; Governato F; Wadsley J; Menci N; Tozzi P; Quinn T; Stadel J; Lake G

Publication date

May 27, 2002

DOI

10.48550/arxiv.astro-ph/0205471

Preprint server

arXiv

Associated Experts

James Wadsley

Professor, Faculty of Science
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Fields of Research (FoR)

5109 Space Sciences51 Physical Sciences
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