Fig. 19
Relation between the cluster mass (M200) and the number of UDGs within the virial radius (R200) in galaxy clusters at 0.044 <z< 0.063 is shown with black points (van der Burg et al. 2016). The red symbols show the same relation for the UDGs with Re> 2.5 kpc. The observed values from our sample are marked with the large symbols, with the extrapolated upper limits shown with the arrows.
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