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Massive stars: stellar models and stellar yields, impact on Galactic Archaeology
Published online by Cambridge University Press: 02 August 2018
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 170 - 177
- Copyright
- Copyright © International Astronomical Union 2018