Fig. 9.
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Normalized SFH-weighted IMF for massive stars that reach TAMS and eventually become RSGs, for a single star population (grey) and from one where binarity is taken into account (orange). For binaries that at some point become RSGs, Minit is calculated based on their MTAMS (Eq. (D.1)), taking into account possible accretion (or merging) during their MS.
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