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Highlights in the Milky Way

Published online by Cambridge University Press:  02 August 2018

Francesca Matteucci ,
Emanuele Spitoni  and
Valeria Grisoni
Francesca Matteucci
Affiliation:
Dipartimento di Fisica, Università di Trieste Via G. Tiepolo 11, 34131 Trieste, Italia email: [email protected]
Emanuele Spitoni
Affiliation:
Dipartimento di Fisica, Università di Trieste Via G. Tiepolo 11, 34131 Trieste, Italia email: [email protected]
Valeria Grisoni
Affiliation:
Dipartimento di Fisica, Università di Trieste Via G. Tiepolo 11, 34131 Trieste, Italia email: [email protected]
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Abstract

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We 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.

Keywords

ISM: abundances - Galaxy: abundances - Galaxy: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 298 - 299
Copyright
Copyright © International Astronomical Union 2018 

References

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