Fig. 4.
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Upper panels: luminosities of H-burning LH (black) and He-burning LHe (red), for the 3 M⊙Z = 10−10 model, during the occurrence of the first dual-shell flash. Right hand panels are a zoomed version of the left panels. Middle panels: convective zones (grey) and H-rich region (blue). Lower panels: logarithm of surface abundances of the most abundant metals.
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