Journal article
The effect of non-gravitational gas heating in groups and clusters of galaxies
Abstract
We present a detailed study of a set of gas-dynamical simulations of galaxy groups and clusters in a flat, Λ-cold dark matter (ΛCDM) model with Ωm= 0.3, aimed at exploring the effect of non-gravitational heating on the observable properties of the intracluster medium (ICM). We use gasoline, a version of the code pkdgrav that includes a smoothed particle hydrodynamics description of hydrodynamics to simulate the formation of four haloes with …
Authors
Borgani S; Governato F; Wadsley J; Menci N; Tozzi P; Quinn T; Stadel J; Lake G
Journal
Monthly Notices of the Royal Astronomical Society, Vol. 336, No. 2, pp. 409–424
Publisher
Oxford University Press (OUP)
Publication Date
October 21, 2002
DOI
10.1046/j.1365-8711.2002.05746.x
ISSN
0035-8711