Fig. 11
The age at which a star terminates the AGB is shown as a function of the initial main sequence stellar mass for three metallicities of 0.019 (long-dashed line, red), 0.008 (Solar metallicity; continuous line, black) and 0.004 (approximately LMC metallicity; short-dashed line, blue). The curves are derived from the stellar evolution tracks of Girardi et al. (2000).
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