Proc. IAU volume 13, issue S334, P166-169 2017 DOI: 10.1017/s1743921317007906 View full text
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P. E. Nissen, V. Silva Aguirre, J. Christensen-Dalsgaard, R. Collet, F. Grundahl, D. Slumstrup

Abstract: AbstractHigh-precision abundances of elements have been derived from HARPS-N spectra of F and G main-sequence stars having ages determined from oscillation frequencies delivered by the Kepler mission. The tight relations between abundance ratios of refractory elements, e.g., [Mg/Fe] and [Y/Mg], and stellar age previously found for solar twin stars are confirmed. These relations provide new information on nucleosynthesis and Galactic evolution. Abundance ratios between volatile and refractory elements, e.g., [C…

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