volume 13, issue S334, P170-177 2017
DOI: 10.1017/s1743921317010808
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Georges Meynet, Arthur Choplin, Sylvia Ekström, Cyril Georgy

Abstract: The physics of massive stars depends (at least) on convection, mass loss by stellar winds, rotation, magnetic fields and multiplicity. We briefly discuss the impact of the first three processes on the stellar yields trying to identify some guidelines for future works.