Explaining the high nitrogen abundances observed in high-z galaxies via population III stars of a few thousand solar masses

Fuente: arXiv

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Bibliographic Details
Main Authors:	Nandal, Devesh, Regan, John A., Woods, Tyrone E., Farrell, Eoin, Ekström, Sylvia, Meynet, Georges
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2402.03428