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Table · dataset · 2012

s-process in low-metallicity stars. II.

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High-resolution spectroscopic observations of 100 metal-poor carbon and s-rich stars (CEMP-s) collected from the literature are compared with the theoretical nucleosynthesis models of the asymptotic giant branch (AGB) presented in Paper I, Cat.

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J/MNRAS/404/1529.

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/mnras/418/28414 d agoJSON v1
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