Fig. 7.
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Upper panel: expected fates of our model stars at different metallicities, as resulting from the present work (variable composition low-temperature opacities and mass-loss rates from Bloecker 1995). Lower panel: expected fates according to the calculations by Gil-Pons et al. (2018; constant composition low-temperature opacities and mass-loss rates from Vassiliadis & Wood 1993).
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