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Fig. 3
Final overproduction factors [X/Fe] of all stable nuclei with A ≥ 30 (full squares) at the center of our 2 M⊙[Fe/H] = −0.5 model star at the end of core helium burning. The s-only nuclei are shown by red diamonds connected by a solid line. The vertical line depicts the total decay of the s-only nucleus 123Te.
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