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Fig. 12


Cumulative radial distribution of GC candidates in Hydra (dotted red line) and Centaurus (solid blue line) around the central galaxies NGC 3311 and NGC 4696, respectively. We note the more central concentration of the Hydra GCs which is imposed by the observational setup, see also Fig. 2. We furthermore indicate as vertical lines the effective radii of the respective central galaxies.

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