The nebular spectra of SN 2023ixf: A lower mass, partially stripped progenitor may be the result of binary interaction

Fuente: arXiv

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Bibliographic Details
Main Authors:	Michel, Philip D., Mazzali, Paolo A., Perley, Daniel A., Hinds, K-Ryan, Wise, Jacob L.
Format:	Preprint
Published:	2025
Subjects:	High Energy Astrophysical Phenomena Astrophysics of Galaxies Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2503.13017