Buchumschlag

Constraining the CSM structure and progenitor mass-loss history of interacting supernovae through 3D hydrodynamic modeling: The case of SN 2014C

Fuente: arXiv

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Bibliographische Detailangaben
Hauptverfasser:	Orlando, S., Greco, E., Hirai, R., Matsuoka, T., Miceli, M., Nagataki, S., Ono, M., Chen, K. -J., Milisavljevic, D., Patnaude, D., Bocchino, F., Elias-Rosa, N.
Format:	Preprint
Veröffentlicht:	2024
Schlagworte:	High Energy Astrophysical Phenomena
Online-Zugang:	Acceder al recurso
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

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