New 17O+α and 22Ne+α rates increase weak s-process yields by tens of times in Z=10^{-3} stars of 15-30 solar masses.
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Overview of methods and recent developments for deriving s- and r-process components of the proto-solar composition.
citing papers explorer
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The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
New 17O+α and 22Ne+α rates increase weak s-process yields by tens of times in Z=10^{-3} stars of 15-30 solar masses.
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The s- and r- components of the proto-solar composition
Overview of methods and recent developments for deriving s- and r-process components of the proto-solar composition.