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• W3105203704 abstract "Context. Heavy-elements, i.e. those beyond the iron peak, mostly form via two neutron capture processes: the slow (s-) and the rapid (r-) process. Metal-poor stars should contain fewer isotopes that form via the s-process, according to currently accepted theory. It has been shown in several investigations that theory and observation do not agree well, raising questions on the validity of either the methodology or the theory." @default.
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• W3105203704 date "2015-07-01" @default.
• W3105203704 modified "2023-10-06" @default.
• W3105203704 title "A three-dimensional hydrodynamical line profile analysis of iron lines and barium isotopes in HD 140283" @default.
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• W3105203704 doi "https://doi.org/10.1051/0004-6361/201424803" @default.
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