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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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Detalles Bibliográficos
Autores principales:	Michel, Philip D., Mazzali, Paolo A., Perley, Daniel A., Hinds, K-Ryan, Wise, Jacob L.
Formato:	Preprint
Publicado:	2025
Materias:	High Energy Astrophysical Phenomena Astrophysics of Galaxies Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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