activity
20032026
most citedComparing the temperatures of galaxy clusters from hydro-N-body simulations to Chandra and XMM-Newton observations

435 citations · 8.4k across the 140 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

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.CO2016★ 18 cited

On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters

Anna Silvia Baldi, Marco De Petris, Federico Sembolini +3

We present a study on the coherent rotation of the intracluster medium and dark matter components of simulated galaxy clusters extracted from a volume-limited sample of the MUSIC p…

astro-ph.CO2016★ 13 cited

Spectral imaging of galaxy clusters with Planck

H. Bourdin, P. Mazzotta, E. Rasia

The Sunyaev-Zeldovich (SZ) effect is a promising tool for detecting the presence of hot gas out to the galaxy cluster peripheries. We developed a spectral imaging algorithm dedicat…

astro-ph.CO2016★ 78 cited

The Morphologies and Alignments of Gas, Mass, and the Central Galaxies of CLASH Clusters of Galaxies

Megan Donahue, Stefano Ettori, Elena Rasia +10

Morphology is often used to infer the state of relaxation of galaxy clusters. The regularity, symmetry, and degree to which a cluster is centrally concentrated inform quantitative…