activity
19962009
most citedClustering of Galaxy Clusters in CDM Universes

149 citations · 370 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2009

Combining Semi-Analytic Models of Galaxy Formation with Simulations of Galaxy Clusters: the Need for AGN Heating

C. J. Short, P. A. Thomas

We present hydrodynamical N-body simulations of clusters of galaxies with feedback taken from semi-analytic models of galaxy formation. The advantage of this technique is that the…

astro-ph2008★ 30 cited

Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei

C. J. Short, P. A. Thomas

We present hydrodynamical N-body simulations of clusters of galaxies with feedback taken from semi-analytic models of galaxy formation. The advantage of this technique is that the…

astro-ph2007★ 40 cited

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

W. G. Hartley, L. Gazzola, F. R. Pearce +2

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 Un…

astro-ph2000★ 98 cited

Simulations of galaxy formation in a cosmological volume

F. R. Pearce, A. Jenkins, C. S. Frenk +5

We present results of large N-body-hydrodynamic simulations of galaxy formation. Our simulations follow the formation of galaxies in cubic volumes of side 100Mpc, in two versions o…

astro-ph2000★ 149 cited

Clustering of Galaxy Clusters in CDM Universes

J. M. Colberg, S. D. M. White, N. Yoshida +9

We use very large cosmological N--body simulations to obtain accurate predictions for the two-point correlations and power spectra of mass-limited samples of galaxy clusters. We co…

astro-ph1999

The effect of radiative cooling on X-ray emission from clusters of galaxies

F. R. Pearce, H. M. P. Couchman, P. A. Thomas +1

In this paper we use state-of-the-art N-body hydrodynamic simulations of a cosmological volume of side 100Mpc to produce many galaxy clusters simultaneously in both the standard co…