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20042025
most citedOn the nature of hydrostatic equilibrium in galaxy clusters

225 citations · 1.1k across the 14 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2022★ 13 cited

Machine Learning to identify ICL and BCG in simulated galaxy clusters

I. Marini, S. Borgani, A. Saro +4

Nowadays, Machine Learning techniques offer fast and efficient solutions for classification problems that would require intensive computational resources via traditional methods. W…

astro-ph.GA2021★ 17 cited

Velocity dispersion of the brightest cluster galaxies in cosmological simulations

I. Marini, S. Borgani, A. Saro +7

Using the DIANOGA hydrodynamical zoom-in simulation set of galaxy clusters, we analyze the dynamics traced by stars belonging to the Brightest Cluster Galaxies (BCGs) and their sur…

astro-ph.GA2020★ 29 cited

Evolution and Role of Mergers in the BCG-Cluster Alignment. A View from Cosmological Hydro-Simulations

Cinthia Ragone-Figueroa, Gian Luigi Granato, Stefano Borgani +5

Contradictory results have been reported on the time evolution of the alignment between clusters and their Brightest Cluster Galaxy (BCG). We study this topic by analyzing cosmolog…

astro-ph.GA2017★ 17 cited

Feedback and feeding in the context of galaxy evolution with SPICA: direct characterization of molecular outflows and inflows

E. González-Alfonso, L. Armus, F. J. Carrera +28

A far-infrared observatory such as the {\it SPace Infrared telescope for Cosmology and Astrophysics} ({\it SPICA}), with its unprecedented spectroscopic sensitivity, would unveil t…

astro-ph.GA2009★ 14 cited

Two phase galaxy formation: The Evolutionary Properties of Galaxies

M Cook, E Barausse, C Evoli +2

We use our model for the formation and evolution of galaxies within a two-phase galaxy formation scenario, showing that the high-redshift domain typically supports the growth of sp…

astro-ph.GA2009★ 51 cited

Two-Phase Galaxy Formation

M. Cook, A. Lapi, G. L. Granato

We propose and test a scenario for the assembly and evolution of luminous matter in galaxies which substantially differs from that adopted by other semianalytic models. As for the…