190 citations · 611 across the 8 of their papers we have counts for
8 papers
The Origin of Lopsided Satellite Galaxy Distribution in Galaxy Pairs
Chen Chris Gong, Noam I Libeskind, Elmo Tempel +6
It is well known that satellite galaxies are not isotropically distributed among their host galaxies as suggested by most interpretations of the CDM model. One type of anisotrop…
Constrained Local UniversE Simulations: A Local Group Factory
Edoardo Carlesi, Jenny G. Sorce, Yehuda Hoffman +8
Near field cosmology is practiced by studying the Local Group (LG) and its neighbourhood. The present paper describes a framework for simulating the near field on the computer. Ass…
The velocity function in the local environment from LCDM and LWDM constrained simulations
J. Zavala, Y. P. Jing, A. Faltenbacher +4
Using constrained simulations of the local Universe for generic cold dark matter and for 1keV warm dark matter, we investigate the difference in the abundance of dark matter halos…
Secondary infall and dark matter haloes
Y. Ascasibar, Y. Hoffman, S. Gottloeber
We test the Secondary Infall Model (SIM) by direct comparison with the results of N-body simulations. Eight cluster-size and six galactic-size dark matter haloes have been selected…
The dependence on environment of Cold Dark Matter Halo properties
V. Avila-Reese, P. Colin, S. Gottloeber +2
High-resolution LCDM cosmological N-body simulations are used to study the properties of galaxy-size dark halos in different environments (cluster, void, and "field"). Halos in clu…
How far do they go? The outer structure of dark matter halos
F. Prada, A. A. Klypin, E. Simonneau +4
We study the density profiles of collapsed galaxy-size dark matter halos with masses 1e11-5e12 Msun focusing mostly on the halo outer regions from the formal virial radius Rvir up…