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Astronomy and Astrophysics, 457, pp. 21-34, http://dx.doi.org./10.1051/0004-6361:5117
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Astronomy and Astrophysics, 446, pp. 417-428, http://dx.doi.org./10.1051/0004-6361:20053946
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2004 (v1)Conference paper
In the framework of the hierarchical model of structure formation, galaxy clusters form through the accretion and merging of substructures of smaller mass. Our goal is to characterize the physics and dynamics of these processes through the study of merging clusters. For this purpose we have built a sample of 10 low--redshift clusters viewed at...
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