Fig. 11
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Mean photometric metallicity of RRLs versus stellar mass for 14 dwarf galaxies (green circles) and the MW (blue star) from Bellazzini et al. (2025), and for the known dynamical sub-structures analysed in this work (red squares). The dashed black line shows the best fit to the 14 dwarfs from Bellazzini et al. (2025), while the dark and light grey areas indicate the ±1σ and ±2σ regions, respectively.
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