Using six high-resolution dissipationless simulations with a varying box size in a flat Lambda
cold dark matter (ΛCDM) universe, we study the mass and redshift dependence of dark …

We analyze the effect of dissipation on the shapes of dark matter (DM) halos using high-
resolution cosmological gasdynamics simulations of clusters and galaxies in the ΛCDM …

We report on the analysis of a suite of smoothed particle hydrodynamics simulations
(incorporating cooling and star formation) of mergers involving idealized X-ray clusters …

ABSTRACT X-ray images of galaxy clusters often show disturbed structures that are
indications of cluster mergers. To complement our previous work on the dynamical state of …

We present the integrated mass profiles for a sample of ten nearby (), relaxed galaxy
clusters, covering a temperature range of, observed with. The mass profiles were derived …

We present new measurements of dark matter distributions in 25 X-ray luminous clusters by
making a full use of the two-dimensional (2D) weak-lensing signals obtained from high …

Previously, it has been recognized that radio halos in galaxy clusters are preferentially
associated with merging systems, as indicated by substructure in the X-ray images and …

Dynamical state of galaxy clusters is closely related to their observational properties in X-
ray, optical and radio wavelengths. We develop a method to diagnose the substructure and …

Results of a systematic study of substructure in X-ray surface brightness distributions of a
combined sample of 470 REFLEX+ BCS clusters of galaxies are presented. The fully …

We used optical imaging and spectroscopic data to derive substructure estimates for local
Universe (< 0.11) galaxy clusters from two different samples. The first was selected through …