Fig. 1
Initial (Mi) versus final (Mf) mass of single stars that become CO WDs for different TP-AGB models (Sect. 2.1.1). The dotted line shows the results of the Hurley et al. (2000) models, the full line shows the results for the fits to the Karakas et al. (2002) models, and the dashed line shows our model.
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