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• W2003899080 abstract "Context. Many studies on the s-process and, more specifically, on the s-process weak component have been performed so far, but a detailed scrutiny of the impact of the stellar evolution modeling uncertainties on the efficiency of this nucleosynthesis process is still missing." @default.
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• W2003899080 date "2010-11-23" @default.
• W2003899080 modified "2023-10-17" @default.
• W2003899080 title "Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase" @default.
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• W2003899080 doi "https://doi.org/10.1051/0004-6361/201015518" @default.
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