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The bolometric light curve modeling of 98 Type I superluminous supernovae using the magnetar- and the circumstellar interaction models reveals surprisingly high ejecta masses

Fuente: arXiv

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Détails bibliographiques
Auteur principal:	Könyves-Tóth, Réka
Format:	Preprint
Publié:	2025
Sujets:	High Energy Astrophysical Phenomena 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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