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Cool giants and supergiants as probes of the chemical evolution of the Milky Way

Published online by Cambridge University Press:  27 October 2016

Livia Origlia
Livia Origlia*
Affiliation:
INAF - Bologna Observatory, Via Ranzani 1, 40127 Bologna, Italy
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Abstract

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This short review is intended to be a snapshot of some recent observational facts and open questions regarding the study of chemical evolution in the innermost regions of the Milky Way, as traced by spectroscopy of cool giant and supergiant stars.

Keywords

stars: abundanceslate-typesupergiantsGalaxy: abundancesdiskstellar content
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 467 - 469
Copyright
Copyright © International Astronomical Union 2016 

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