Abstract:Context. To study the effects of environment on galaxies, we use H I observations of galaxies in and around the cluster Abell 2626 (A2626). The cluster can effectively be divided into three different environments: the cluster itself, a group environment in the periphery of the cluster (we call it the Swarm), and substructure in the cluster itself. We use these to study the dependence of the galaxy properties on environment.
Aims. We have explored the relation between H I deficiency, H I morphology, and star fo… Show more
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