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Fig. 9.
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Evolution of the abundances and reaction rates in the units of [cm3 s−1 mol−1]: as a function of Ncapt in the large (full lines) and fictitious (dashed lines) networks during the seventh interpulse of a 2 M⊙, [Fe/H] = −2 star. The effective neutron-capture rate of ls, hs, and vhs was multiplied by 10 for readability.
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