687 citations · 2.5k across the 16 of their papers we have counts for
20 papers
Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
Robert P. C. Wiersma, Joop Schaye, Tom Theuns +2
(Abridged) We present an implementation of stellar evolution and chemical feedback for smoothed particle hydrodynamics (SPH) simulations. We consider the timed release of individua…
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…
Evolution of the metal content of the intra-cluster medium with hydrodynamical simulations
D. Fabjan, L. Tornatore, S. Borgani +2
We present a comparison between simulation results and X-ray observational data on the evolution of the metallicity of the intra-cluster medium (ICM). The simulations of galaxy clu…
On the Dynamical Origin of the ICM Metallicity Evolution
S. A. Cora, L. Tornatore, P. Tozzi +1
We present a study on the origin of the metallicity evolution of the intra-cluster medium (ICM) by applying a semi-analytic model of galaxy formation to N-body/SPH (smoothed partic…
The chemical enrichment of the ICM from hydrodynamical simulations
S. Borgani, D. Fabjan, L. Tornatore +3
The study of the metal enrichment of the intra-cluster and inter-galactic media (ICM and IGM) represents a direct means to reconstruct the past history of star formation, the role…
Population III stars: hidden or disappeared ?
L. Tornatore, A. Ferrara, R. Schneider
A PopIII/Pop II transition from massive to normal stars is predicted to occur when the metallicity of the star forming gas crosses the critical range Z_cr = 10^(-5 +/- 1) Z_sun. To…