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The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications
Weiguang Cui, Alexander Knebe, Gustavo Yepes +34
We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…
Colour-magnitude diagram in simulations of galaxy formation
Milena Valentini, Alessandro Bressan, Stefano Borgani +3
State-of-the-art cosmological hydrodynamical simulations have star particles with typical mass between and M according to resolution, and treat th…
Dust Evolution in Galaxy Cluster Simulations
Eda Gjergo, Gian Luigi Granato, Giuseppe Murante +3
We implement a state-of-the-art treatment of the processes affecting the production and Interstellar Medium (ISM) evolution of carbonaceous and silicate dust grains within SPH simu…
BCG Mass Evolution in Cosmological Hydro-Simulations
C. Ragone-Figueroa, G. L. Granato, M. E. Ferraro +5
We analyze the stellar growth of Brightest Cluster Galaxies (BCGs) produced by cosmological zoom-in hydrodynamical simulations of the formation of massive galaxy clusters. The evol…
Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
Nhut Truong, Elena Rasia, Veronica Biffi +7
Recent X-ray observations of galaxy clusters show that the distribution of intra-cluster medium (ICM) metallicity is remarkably uniform in space and time. In this paper, we analyse…
The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
Veronica Biffi, Susana Planelles, Stefano Borgani +4
The uniformity of the intra-cluster medium (ICM) enrichment level in the outskirts of nearby galaxy clusters suggests that chemical elements were deposited and widely spread into t…