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Selected topics in the evolution of low-mass stars

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Figure

Figure 1. H-R diagram showing the evolution of a low-mass star with the following parameters:The main evolutionary stages are labeled, and key stages in the star’s life are numbered as follows: (1) ZAMS; (2)central H exhaustion and turn-off point; (3) first
Figure 2. As in Figure 1, but zooming in on the main nuclear burning stages.
Figure 4. Evolution of the recommended solar metal abundancein Z⊙. The gray arrows point to the possible increase Z⊙ due to the inclusion of MHD effects, as recently suggested by Fabbian et al
Figure 5. Chemical evolution models for two GCs, namely M13 (NGC 6205,[O/Fe]. Note the differentlines solid lines) and NGC 2808 (dashed)

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