Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …

One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …

In the outer regions of a galaxy cluster, galaxies either may be falling into the cluster for the
first time or have already passed through the cluster centre at some point in their past. To …

We study the connection between morphology and dynamical state of the simulated galaxy
clusters in z∈[0, 1.031] from The Three Hundred project. We quantify cluster dynamical state …

The distribution of baryons provides a significant way to understand the formation of galaxy
clusters by revealing the details of its internal structure and changes over time. In this paper …

The effect of galactic orbits on a galaxy's internal evolution within a galaxy cluster
environment has been the focus of heated debate in recent years. To understand this …

Galaxy cluster outskirts are described by complex velocity fields induced by diffuse material
collapsing towards filaments, gas, and galaxies falling into clusters, and gas shock …

Upcoming wide-field surveys are well suited to studying the growth of galaxy clusters by
tracing galaxy and gas accretion along cosmic filaments. We use hydrodynamic simulations …

Accurate and precise measurement of the masses of galaxy clusters is key to deriving robust
constraints on cosmological parameters. However, increasing evidence from observations …

In this work, we combine the semi-analytic model of galaxy formation and evolution sag with
the 102 relaxed simulated galaxy clusters from the three hundred project, and we study the …