Stellar mass distribution of the present-day population of TP-AGB stars relative to the total number of TP-AGB stars for the duration of the TP-AGB phase from Ferrarotti & Gail (2006) (thick line). Shaded area shows variations due to uncertainties in star formation history. Results calculated for the durations from Marigo & Girardi (2007) and Hurley et al. (2000) are shown for comparison (dark green and light blue lines, respectively).
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