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20112017
most citedConnecting Angular Momentum and Galactic Dynamics: The complex Interplay between Spin, Mass, and Morphology

266 citations · 1.7k across the 26 of their papers we have counts for

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Showing astro-ph.COShow all

14 papers · 1 filter

astro-ph.CO2017★ 21 cited

Simulations of the Galaxy Cluster CIZA J2242.8+5301 I: Thermal Model and Shock Properties

J. M. F. Donnert, A. M. Beck, K. Dolag +1

The giant radio relic in CIZA J2242.8+5301 is likely evidence of a Mpc sized shock in a massive merging galaxy cluster. However, the exact shock properties are still not clearly de…

astro-ph.CO2017★ 97 cited

The history of chemical enrichment in the intracluster medium from cosmological simulations

V. Biffi, S. Planelles, S. Borgani +8

The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the connection with the cosmic sta…

astro-ph.CO2016★ 102 cited

Pressure of the hot gas in simulations of galaxy clusters

S. Planelles, D. Fabjan, S. Borgani +11

We analyze the radial pressure profiles, the ICM clumping factor and the Sunyaev-Zel'dovich (SZ) scaling relations of a sample of simulated galaxy clusters and groups identified in…

astro-ph.CO2016★ 111 cited

Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution

N. Truong, E. Rasia, P. Mazzotta +11

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity,…

astro-ph.CO2016★ 225 cited

On the nature of hydrostatic equilibrium in galaxy clusters

V. Biffi, S. Borgani, G. Murante +7

In this paper we investigate the level of hydrostatic equilibrium (HE) in the intra-cluster medium of simulated galaxy clusters, extracted from state-of-the-art cosmological hydrod…

astro-ph.CO2015★ 60 cited

nIFTy galaxy cluster simulations II: radiative models

Federico Sembolini, Pascal Jahan Elahi, Frazer R. Pearce +19

We have simulated the formation of a massive galaxy cluster (M = 1.110) in a CDM universe using 10 different codes (RAMSES, 2 in…