Proc. IAU volume 13, issue S334, P298-299 2017 DOI: 10.1017/s174392131700789x View full text
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Francesca Matteucci, Emanuele Spitoni, Valeria Grisoni

Abstract: AbstractWe discuss some important topics concerning the chemical evolution of the Milky Way. In particular, we compare the predictions of theoretical chemical models for our Galaxy with the latest observational data in order to derive constraint on the formation and evolution of the various Galactic components.