Fig. 18
Spectroscopically confirmed star clusters (crosses) of the Hydra Cluster (Misgeld et al. 2011) overlaid on a DSS2 image of the Hydra Cluster. Only those clusters which are located within the two HST WFPC2 fields (marked by grey lines) have measured sizes. The black circles indicate projected distances from the central galaxy NGC 3311 of 50, 100, and 200 kpc.
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