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astro-ph2000

Public Release of N-body simulation and related data by the Virgo consortium

C. S. Frenk, J. M. Colberg, H. M. P. Couchman +10

We are making available on the WWW a selection of the archived data from N-body simulations carried out by the Virgo consortium and related groups. This currently includes: (i) tim…

astro-ph2000

High Resolution Simulation of Galaxy Formation with Feedback

R. J. Thacker, H. M. P. Couchman

We present results from a Smoothed Particle Hydrodynamic (SPH) simulation of galaxy formation that exceeds the minimum resolution requirement suggested by Steinmetz & Muller (1993)…

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…

astro-ph1999

Galaxy clustering determined from numerical cosmological simulations

Adrian Jenkins, C. S. Frenk, F. R. Pearce +7

We have simulated the growth of structure in two 100 Mpc boxes for LCDM and SCDM universes. These N-body/SPH simulations include a gaseous component which is able to cool radiative…

astro-ph1999

Cosmological galaxy formation

F. R. Pearce, C. S. Frenk, A. Jenkins +7

We discuss the first results from two successful simulations of galaxy formation within a cosmological volume. With over 2000 large objects forming in each we have sufficient numbe…

astro-ph1998

Galaxy Clusters in the Hubble Volume Simulations

Joerg M. Colberg, Simon D. M. White, Thomas J. MacFarland +8

We report on analyses of cluster samples obtained from the Hubble Volume Simulations. These simulations, an model named CDM and a flat low model with a cosmological co…