Fig. 5

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Nuclear star cluster effective radius (reff) versus stellar mass . The colour-coding and symbols are the same as in Fig. 4. Note that compared to Fig. 4 fewer NSCs are shown because of a lack of measured effective radii for the dwarf galaxy sample in the core of the Virgo cluster (Sánchez-Janssen et al. 2019; Ferrarese et al. 2020). Uncertainties are omitted for clarity.
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