108 citations · 271 across the 5 of their papers we have counts for
5 papers
Simulating the formation of a proto-cluster at z~2
A. Saro, S. Borgani, L. Tornatore +3
We present results from two high-resolution hydrodynamical simulations of proto-cluster regions at z~2.1. The simulations have been compared to observational results for the socall…
Star formation and bar instability in cosmological haloes
Anna Curir, Paola Mazzei, Giuseppe Murante
This is the third of a series of papers presenting the first attempt to analyze the growth of the bar instability in a consistent cosmological scenario. In the previous two article…
Evolution of stellar-gaseous disks in cosmological haloes
A. Curir, P. Mazzei, G. Murante
We explore the growth and the evolution of the bar instability in stellar-gaseous disks embedded in a suitable dark matter halo evolving in a fully consistent cosmological framewor…
Diffuse stellar component in galaxy clusters and the evolution of the most massive galaxies at z<~1
Pierluigi Monaco, Giuseppe Murante, Stefano Borgani +1
The high end of the stellar mass function of galaxies is observed to have little evolution since z~1. This represents a stringent constraint for merger--based models, aimed at expl…
Simulated X-ray galaxy clusters at the virial radius: slopes of the gas density, temperature and surface brightness profiles
M. Roncarelli, S. Ettori, K. Dolag +3
Using a set of hydrodynamical simulations of 9 galaxy clusters with masses in the range 1.5 10^{14} M_sun < M_vir < 3.4 10^{15} M_sun, we have studied the density, temperature and…