activity
20202026
most citedOn the accretion history of galaxy clusters: temporal and spatial distribution

33 citations · 120 across the 18 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.CO2024★ 8 cited

Turbulent Pressure Support in Galaxy Clusters -- Impact of the Hydrodynamical Solver

Frederick Groth, Milena Valentini, Ulrich P. Steinwandel +2

The amount of turbulent pressure in galaxy clusters is still debated, especially as for the impact of the dynamical state and the hydro-method used for simulations. We study the tu…

astro-ph.IM2024★ 7 cited

Vortex-p: a Helmholtz-Hodge and Reynolds decomposition algorithm for particle-based simulations

David Vallés-Pérez, Susana Planelles, Vicent Quilis +3

Astrophysical turbulent flows display an intrinsically multi-scale nature, making their numerical simulation and the subsequent analyses of simulated data a complex problem. In par…

astro-ph.CO2024★ 5 cited

Cosmic accretion shocks as a tool to measure the dark matter mass of galaxy clusters

David Vallés-Pérez, Vicent Quilis, Susana Planelles

Cosmological accretion shocks created during the formation of galaxy clusters are a ubiquitous phenomenon all around the Universe. These shocks, and their features, are intimately…

astro-ph.CO2024★ 4 cited

Density Fluctuations in the Intracluster Medium: An Attempt to Constrain Viscosity with Cosmological Simulations

Tirso Marin-Gilabert, Ulrich P. Steinwandel, Milena Valentini +2

The impact of viscosity in the Intracluster Medium (ICM) is still an open question in astrophysics. To address this problem, we have run a set of cosmological simulations of three…

astro-ph.CO2024★ 3 cited

The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect

Óscar Monllor-Berbegal, David Vallés-Pérez, Susana Planelles +1

Forthcoming measurements of the Sunyaev-Zeldovich (SZ) effect in galaxy clusters will dramatically improve our understanding of the main intra-cluster medium (ICM) properties and h…