Massive stars evolution: feedbacks in low-Z environment. (arXiv:1911.01771v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Ekstrom_S/0/1/0/all/0/1">Sylvia Ekstr&#xf6;m</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Meynet_G/0/1/0/all/0/1">Georges Meynet</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Georgy_C/0/1/0/all/0/1">Cyril Georgy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Groh_J/0/1/0/all/0/1">Jos&#xe9; Groh</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Choplin_A/0/1/0/all/0/1">Arthur Choplin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Song_H/0/1/0/all/0/1">Hanfeng Song</a>

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.

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.

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