activity
19942007
most citedThe Importance of Mergers for the Origin of Intracluster Stars in Cosmological Simulations of Galaxy Clusters

269 citations · 908 across the 8 of their papers we have counts for

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Showing 2007Show all

8 papers · 1 filter

astro-ph200730 cited

How does gas cool in DM halos?

M. Viola, P. Monaco, S. Borgani +2

In order to study the process of cooling in dark-matter (DM) halos and assess how well simple models can represent it, we run a set of radiative SPH hydrodynamical simulations of i…

astro-ph200753 cited

Joint deprojection of Sunyaev-Zeldovich and X-ray images of galaxy clusters

S. Ameglio, S. Borgani, E. Pierpaoli +1

We present two non-parametric deprojection methods aimed at recovering the three-dimensional density and temperature profiles of galaxy clusters from spatially resolved thermal Sun…

astro-ph200782 cited

X-MAS2: Study Systematics on the ICM Metallicity Measurements

E. Rasia, P. Mazzotta, H. Bourdin +5

(Abridged)The X-ray measurements of the ICM metallicity are becoming more frequent due to the availability of powerful X-ray telescope with excellent spatial and spectral resolutio…

astro-ph2007372 cited

Chemical enrichment of galaxy clusters from hydrodynamical simulations

L. Tornatore, S. Borgani, K. Dolag +1

We present cosmological hydrodynamical simulations of galaxy clusters aimed at studying the process of metal enrichment of the intra--cluster medium (ICM). These simulations have b…

astro-ph2007260 cited

The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample

H. Boehringer, P. Schuecker, G. W. Pratt +31

The largest uncertainty for cosmological studies using clusters of galaxies is introduced by our limited knowledge of the statistics of galaxy cluster structure, and of the scaling…

astro-ph2007

Evolution in the iron abundance of the ICM

I. Balestra, P. Tozzi, S. Ettori +4

We present a Chandra analysis of the X-ray spectra of 56 clusters of galaxies at , which cover a temperature range of keV. Our analysis is aimed at measuring th…