A classification of the galaxy cluster's dynamical state is crucial when dealing with large
samples. The identification of the most relaxed and most disturbed objects is necessary for …

We use a set of about 300 simulated clusters from the three hundred Project to calculate
their hydrostatic masses and evaluate the associated bias by comparing them with the true …

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 …

Context. The characterization of the dynamical state of galaxy clusters is key to studying their
evolution, evaluating their selection, and using them as a cosmological probe. In this …

The relationship linking a galaxy cluster's total mass with the concentration of its mass profile
and its redshift is a fundamental prediction of the Cold Dark Matter (CDM) paradigm of …

Matter distribution around clusters is highly anisotropic because clusters are the nodes of
the cosmic web. The shape of the clusters and the number of filaments to which they are …

Theoretical and observational studies have suggested that ram-pressure stripping (RPS) by
the intracluster medium can be enhanced during cluster interactions, boosting the formation …

Matter distribution in the environment of galaxy clusters, from their cores to their connected
cosmic filaments, must in principle be related to the underlying cluster physics and its …

While awaiting direct velocity measurements of gas motions in the hot intracluster medium,
we rely on indirect probes, including gas perturbations in galaxy clusters. Using a sample …

The intra-cluster medium is prone to turbulent motion that will contribute to the non-thermal
heating of the gas, complicating the use of galaxy clusters as cosmological probes. Indirect …