Dwarf galaxies in the MATLAS survey: Hubble Space Telescope observations of nuclear star clusters

Open Access

Fig. 6.

M $_{*}^{GC}$ $_{\ast}^{\mathrm{GC}}$ as a function of the radial distribution of the GCs for the nucleated (black) and non-nucleated (green) dwarfs. We show the running average of the radial distance δ_GC per bin 0.5 log(M $_{*}^{NSC}$ $_{\ast}^{\mathrm{NSC}}$ /M_⊙) with lines. The error bars represent the standard deviation.

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