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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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Détails bibliographiques
Auteurs principaux:	Michel, Philip D., Mazzali, Paolo A., Perley, Daniel A., Hinds, K-Ryan, Wise, Jacob L.
Format:	Preprint
Publié:	2025
Sujets:	High Energy Astrophysical Phenomena Astrophysics of Galaxies Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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