We search for and characterize substructures in the projected distribution of galaxies observed in the wide field CCD images of the 77 nearby clusters of the WIde-field Nearby Galaxy-cluster Survey (WINGS). This sample is complete in X-ray flux in the redshift range 0.04<z<0.07. We search for substructures in WINGS clusters with DEDICA, an adaptive-kernel procedure. We test the procedure on Monte-Carlo simulations of the observed frames and determine the reliability for the detected structures. DEDICA identifies at least one reliable structure in the field of 55 clusters. 40 of these clusters have a total of 69 substructures at the same redshift of the cluster (redshift estimates of substructures are from color-magnitude diagrams). The frac...
Complementary one-, two-, and three-dimensional tests for detecting the presence of substructure in ...
This is the first paper of a series that will present data and scientific results from the WINGS pro...
Context. To effectively investigate galaxy formation and evolution, it is of paramount importance to...
Aims.We search for and characterize substructures in the projected distribution of galaxies observed...
In this Thesis different observational and theoretical aspects related to the dynamics of galaxy clu...
International audienceContext. The DAFT/FADA survey is based on the study of similar to 90 rich (mas...
Context. We study the distribution of galaxies in nearby clusters to shed light on the evolutionary ...
Context. According to the current cosmological paradigm, large scale structures form hierarchically ...
Context. The DAFT/FADA survey is based on the study of ~90 rich (masses found in the liter...
We present the results from a comprehensive spectroscopic survey of the WINGS (WIde-field Nearby Gal...
International audienceContext. We study the distribution of galaxies in nearby clusters to shed ligh...
Aims: We present the results from a comprehensive spectroscopic survey of the WINGS (WIde-field Near...
We present a new method to quantify substructures in clusters of galaxies, based on the analysis of ...
Complementary one-, two- and three-dimensional tests for detecting the presence of substructure in c...
Abstract. WINGS is a two-band (B and V), wide-field imaging survey of a com-plete, all-sky X-ray sel...
Complementary one-, two-, and three-dimensional tests for detecting the presence of substructure in ...
This is the first paper of a series that will present data and scientific results from the WINGS pro...
Context. To effectively investigate galaxy formation and evolution, it is of paramount importance to...
Aims.We search for and characterize substructures in the projected distribution of galaxies observed...
In this Thesis different observational and theoretical aspects related to the dynamics of galaxy clu...
International audienceContext. The DAFT/FADA survey is based on the study of similar to 90 rich (mas...
Context. We study the distribution of galaxies in nearby clusters to shed light on the evolutionary ...
Context. According to the current cosmological paradigm, large scale structures form hierarchically ...
Context. The DAFT/FADA survey is based on the study of ~90 rich (masses found in the liter...
We present the results from a comprehensive spectroscopic survey of the WINGS (WIde-field Nearby Gal...
International audienceContext. We study the distribution of galaxies in nearby clusters to shed ligh...
Aims: We present the results from a comprehensive spectroscopic survey of the WINGS (WIde-field Near...
We present a new method to quantify substructures in clusters of galaxies, based on the analysis of ...
Complementary one-, two- and three-dimensional tests for detecting the presence of substructure in c...
Abstract. WINGS is a two-band (B and V), wide-field imaging survey of a com-plete, all-sky X-ray sel...
Complementary one-, two-, and three-dimensional tests for detecting the presence of substructure in ...
This is the first paper of a series that will present data and scientific results from the WINGS pro...
Context. To effectively investigate galaxy formation and evolution, it is of paramount importance to...