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Rapidly rotating Population III stellar models as a source of primary nitrogen

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Tsiatsiou, Sophie, Sibony, Yves, Nandal, Devesh, Sciarini, Luca, Hirai, Yutaka, Ekstrom, Sylvia, Farrell, Eoin, Murphy, Laura, Choplin, Arthur, Hirschi, Raphael, Chiappini, Cristina, Liu, Boyuan, Bromm, Volker, Groh, Jose, Meynet, Georges
Formato:	Preprint
Publicado:	2024
Materias:	Solar and Stellar Astrophysics Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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