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Fig. 6.
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Evolution of the surface mass fraction of 27Al (top panels) and 28Si (bottom) as a function of the (current) stellar mass of the Z = 3 × 10−5 (left) and Z = 3 × 10−7 (right) model stars. The colour-coding is the same as in Fig. 4. Red arrows on the left side of each pane indicate the initial mass fractions.
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