activity
19972007
most citedThe redshift dependence of the structure of massive LCDM halos

510 citations · 887 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

11 papers · 1 filter

astro-ph2007510 cited

The redshift dependence of the structure of massive LCDM halos

Liang Gao, Julio F. Navarro, Shaun Cole +5

(Abridged) We use two very large cosmological simulations to study how the density profiles of relaxed LCDM dark halos depend on redshift and on halo mass. We confirm that these pr…

astro-ph2007370 cited

Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology

A. E. Evrard, J. Bialek, M. Busha +14

We present a precise estimate of the bulk virial scaling relation of halos formed via hierarchical clustering in an ensemble of simulated cold dark matter cosmologies. The result i…

astro-ph20047 cited

Disk Galaxy Rotation Curves in Triaxial CDM Halos

E. Hayashi, J. F. Navarro, A. Jenkins +7

We use N-body hydrodynamical simulations to study the structure of disks in triaxial potentials resembling CDM halos. Our analysis focuses on the accuracy of the dark mass distribu…

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-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…