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Fig. 8.
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Slope of the IGIMF in the stellar mass range [0.4, 0.8] M⊙ for all models displayed in Fig. 7. Additional models with an SFR = 10−4 M⊙ yr−1 as well as with a = 1.5 are included. The observational data points correspond to six UFD satellites of the Milky Way and are taken from Gennaro et al. (2018).
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