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The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
Gian Luigi Granato, Cinthia Ragone-Figueroa, Rosa Dominguez-Tenreiro +4
We compute and study the infrared and sub-mm properties of high redshift () simulated clusters and proto-clusters. The results of a large set of hydro-dynamical zoom-i…
Temperature Structure of the Intra-Cluster Medium from SPH and AMR simulations
Elena Rasia, Erwin T. Lau, Stefano Borgani +8
Analyses of cosmological hydrodynamic simulations of galaxy clusters suggest that X-ray masses can be underestimated by 10% to 30%. The largest bias originates by both violation of…
The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
A. Obreja, C. B. Brook, G. Stinson +4
Using cosmological galaxy simulations from the MaGICC project, we study the evolution of the stellar masses, star formation rates and gas phase abundances of star forming galaxies.…
Black hole accretion preferentially occurs in gas rich galaxies
Fabio Vito, Roberto Maiolino, Paola Santini +15
We have investigated the gas content of a sample of several hundred AGN host galaxies at z1 and compared it with a sample of inactive galaxies, matched in bins of stellar mass a…