Chemical evolution of ultra-faint dwarf galaxies in the self-consistently calculated integrated galactic IMF theory

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Fig. 9.

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SFH requiring an artificial gas-cooling time. The blue dashed line is the same as in Fig. 1. Compared to the best-fit IGIMF-R14 model (with the SFH shown in Fig. 1), the discretised SFH has a larger spread but similar galaxy evolution results (see Sect. 7.5).

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