Fig. 9.
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Estimates of the number of PS stars that can be found at different mass ranges (left) and different luminosity ranges(right) at SMC (upper) and LMC (middle) and solar (lower) metallicities. Values above the bars in the upper right panel show the percentage of puffed-up stripped stars relative to the number of all stars in that luminosity bin, most of which are MS, based on Schootemeijer et al. (2021).
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