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Fig. 5.
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M/LV of the DF2 clusters compared to Milky Way GCs (grey) for distances of 16.2 Mpc (black circles) and 21.7 Mpc (orange triangles). In general, the DF2 GCs fall below the Milky Way sample if the larger distance is assumed. The most luminous Milky Way GC with M/LV ∼ 2.5 is ω Cen (NGC 5139).
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