Based on optical data we propose a dynamycal model for A115. From spatial and radial velocity distributions we find three massive subsclusters that configure a pre-merging scenario. On this basis, we discuss on the origin of the radio emission and its correlation with X-rays.
The Internal Dynamics of A115 Nearby Cluster of GalaxiesGroups of Galaxies in the Nearby Universe
GIRARDI, MARISA
2007-01-01
Abstract
Based on optical data we propose a dynamycal model for A115. From spatial and radial velocity distributions we find three massive subsclusters that configure a pre-merging scenario. On this basis, we discuss on the origin of the radio emission and its correlation with X-rays.File in questo prodotto:
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