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Fig. 11


Mass budget within R ≃ 3 h in different types of dwarf galaxies: Irrs (blue diamonds, from Swaters et al. 2009), BCDs (black squares, from Lelli et al. 2014b), and TDGs (red points). For Irrs Mbar is estimated assuming both a “heavy disc” with (open symbols) and a “light disc” with (filled symbols). For BCDs the stellar mass is estimated from colour-magnitude diagrams of resolved stellar populations (see Lelli et al. 2014b).

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