Explaining the $^{12}\text{C}/^{13}\text{C}$ ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars

Fuente: arXiv

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Bibliographic Details
Main Authors:	Rizzuti, F., Cescutti, G., Molaro, P., Roberti, L., Chieffi, A., Limongi, M., Magrini, L., Matteucci, F.
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2503.20876