Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S334(13), p. 298-299
DOI: 10.1017/s174392131700789x
Full text: Unavailable
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.