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This article has an erratum: [https://doi.org/10.1051/0004-6361/202451953e]


Fig. 11.

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log M – log ΣM relation for star-forming complexes (purple). Dashed line traces the 5% percentile of log ΣM for globular clusters and ultra-compact dwarfs. Red and black contours trace the distributions of local dwarf spheroidals from Norris et al. (2014) Fornax dwarf galaxies from Venhola et al. (2018, 2022).

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