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20022008
most citedDiscovery of diffuse radio emission at the center of the most X-ray-luminous cluster RX J1347.5-1145

75 citations · 156 across the 3 of their papers we have counts for

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astro-ph200868 cited

On the influence of ram-pressure stripping on interacting galaxies in clusters

W. Kapferer, T. Kronberger, C. Ferrari +2

We investigate the influence of ram pressure on the star-formation rate and the distribution of gas and stellar matter in interacting model galaxies in clusters. To simulate the ba…

astro-ph200775 cited

Discovery of diffuse radio emission at the center of the most X-ray-luminous cluster RX J1347.5-1145

Myriam Gitti, Chiara Ferrari, Wilfried Domainko +2

We report on new VLA radio observations of the distant cluster RX J1347.5-1145, which is the most luminous in X-rays. We aim at investigating the possible presence of diffuse and e…

astro-ph200613 cited

ATCA observations of the galaxy cluster Abell 3921 - I. Radio emission from the central merging sub-clusters

C. Ferrari, R. W. Hunstead, L. Feretti +2

We present the analysis of our 13 and 22 cm ATCA observations of the central region of the merging galaxy cluster A3921 (z=0.094). We investigated the effects of the major merger b…

astro-ph2005

Chandra observation of the multiple merger cluster Abell 521

C. Ferrari, M. Arnaud, S. Ettori +2

We present the Chandra analysis of the galaxy cluster A521 (z=0.247). The high resolution of the Chandra observation has allowed us to refine the original merging scenario proposed…

astro-ph2003

Galaxy Alignments as a Probe of the Dynamical State of Clusters

M. Plionis, C. Benoist, S. Maurogordato +2

We present indications, based on a sample of 303 Abell clusters, for a relation between the dynamical state of clusters and the alignments of galaxy members with their parent clust…

astro-ph2002

Multiple merging events in Abell 521

C. Ferrari, S. Maurogordato, A. Cappi +1

We present a detailed spatial and dynamical analysis of the central ~2.2~\h~Mpc region of the galaxy cluster Abell~521 (z=0.247), based on 238 spectra obtained at the 3.6~m T…