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• W2126331421 abstract "From newly obtained high-resolution, high signal-to-noise ratio spectra the abundances of the elements La and Eu have been determined over the stellar metallicity range -3 < [Fe/H] < +0.3 in 159 giant and dwarf stars. Lanthanum is predominantly made by the s-process in the solar system, while Eu owes most of its solar system abundance to the r-process. The changing ratio of these elements in stars over a wide metallicity range traces the changing contributions of these two processes to the Galactic abundance mix. Large s-process abundances can be the result of mass transfer from very evolved stars, so to identify these cases we also report carbon abundances in our metal-poor stars. Results indicate that the s-process may be active as early as [Fe/H] = -2.6, although we also find that some stars as metal-rich as [Fe/H] = -1 show no strong indication of s-process enrichment. There is a significant spread in the level of s-process enrichment even at solar metallicity." @default.
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• W2126331421 date "2004-12-20" @default.
• W2126331421 modified "2023-10-05" @default.
• W2126331421 title "The Rise of the<i>s</i>‐Process in the Galaxy" @default.
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• W2126331421 doi "https://doi.org/10.1086/424504" @default.
• W2126331421 hasPublicationYear "2004" @default.
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