Fig. 3.
Upper panel: mass of the stellar models at He ignition for the different initial chemical compositions computed in this work. Lower panel: same as upper panel but for the works of Xiong et al. (2017) (X+2016) and Miller Bertolami et al. (2008) (MB+2008) for Z = 0.02; and Castellani et al. (2006) (Castellani+2006) and Cassisi et al. (2003) (Cassisi+2003) for Z = 0.0015.
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