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Massive star evolution: feedbacks in low-Z environment

Published online by Cambridge University Press:  30 October 2019

Sylvia Ekström Open the ORCID record for Sylvia Ekström [Opens in a new window] ,
Georges Meynet ,
Cyril Georgy Open the ORCID record for Cyril Georgy [Opens in a new window] ,
José Groh ,
Arthur Choplin  and
Hanfeng Song
Sylvia Ekström
Affiliation:
Department of Astronomy, University of Geneva, Maillettes 51, CH-1290, Versoix, Switzerland email: sylvia.ekstrom@unige.ch
Georges Meynet
Affiliation:
Department of Astronomy, University of Geneva, Maillettes 51, CH-1290, Versoix, Switzerland email: sylvia.ekstrom@unige.ch
Cyril Georgy
Affiliation:
Department of Astronomy, University of Geneva, Maillettes 51, CH-1290, Versoix, Switzerland email: sylvia.ekstrom@unige.ch
José Groh
Affiliation:
Trinity College, University of Dublin, Dublin 2, Republic of Ireland
Arthur Choplin
Affiliation:
Department of Astronomy, University of Geneva, Maillettes 51, CH-1290, Versoix, Switzerland email: sylvia.ekstrom@unige.ch
Hanfeng Song
Affiliation:
College of Physics, Guizhou University, Guiyang City, 550025 Guizhou Province, PR China
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Abstract

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Massive stars are the drivers of the chemical evolution of dwarf galaxies. We review here the basics of massive star evolution and the specificities of stellar evolution in low-Z environment. We discuss nucleosynthetic aspects and what observations could constrain our view on the first generations of stars.

Keywords

stars: evolutionstars: early-typenucleosynthesisgalaxies: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S344: Dwarf Galaxies: From the Deep Universe to the Present , August 2018 , pp. 153 - 160
Copyright
© International Astronomical Union 2019 

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