Fig. 6.
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Theoretical and observed luminosity functions of RSGs from Y23. We limit our comparison to systems that eventually result in a FeCC, and for which log10(Lmin/L⊙) > Lmin, and Teff < Teff, max. The top x-axis shows the corresponding initial mass of models with an average RSG luminosity of the bottom x-axis, according to Eq. (A.1) following the best-fit parameters for ṀY23.
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