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19942008
most citedGiant Ringlike Radio Structures Around Galaxy Cluster Abell 3376

187 citations · 820 across the 25 of their papers we have counts for

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49 papers · 1 filter

astro-ph200815 cited

An analysis of electron distributions in galaxy clusters by means of the flux ratio of iron lines FeXXV and XXVI

D. A. Prokhorov, F. Durret, V. A. Dogiel +1

The interpretation of hard X-ray emission from galaxy clusters is still ambiguous and different models proposed can be probed using various observational methods. Here we explore a…

astro-ph200811 cited

On the nature of faint Low Surface Brightness galaxies in the Coma cluster

C. Adami, R. Pello, M. P. Ulmer +5

This project is the continuation of our study of faint Low Surface Brightness Galaxies (fLSBs) in one of the densest nearby galaxy regions known, the Coma cluster. Our goal is to i…

astro-ph20088 cited

The optical/X-ray connection: ICM iron content and galaxy optical luminosity in 20 galaxy clusters

T. F. Lagana, R. A. Dupke, L. Sodre +2

X-ray observations of galaxy clusters have shown that the intra-cluster gas has iron abundances of about one third of the solar value. These observations also show that part (if no…

astro-ph200834 cited

Galaxy evolution in Abell 85: I. Cluster substructure and environmental effects on the blue galaxy population

H. Bravo-Alfaro, C. A. Caretta, C. Lobo +2

This series of papers explores the evolution of late-type galaxies in the rich cluster Abell 85. Here, we revisit the complex dynamical state of A 85 by using independent methods.…

astro-ph20089 cited

Orientations of very faint galaxies in the Coma cluster

C. Adami, R. Gavazzi, J. C. Cuillandre +5

We have then searched for preferential orientations of faint galaxies in the Coma cluster (down I_Vega~-11.5). By applying a deconvolution method to deep u* and I band images of th…

astro-ph200825 cited

Photometric redshifts as a tool to study the Coma cluster galaxy populations

C. Adami, O. Ilbert, R. Pello +5

We investigate the Coma cluster galaxy luminosity function (GLF) at faint magnitudes, in particular in the u* band by applying photometric redshift techniques applied to deep u*, B…