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Hydrogen-Poor Superluminous Supernovae in the Nebular Phase: Spectral Diversity Due to Ejecta Ionization as a Probe of the Power Source

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Blanchard, Peter K., Berger, Edo, Gomez, Sebastian, Nicholl, Matt, Chornock, Ryan, Kumar, Harsh, Margutti, Raffaella, Hiramatsu, Daichi, Sears, Huei
Formato:	Preprint
Publicado:	2025
Materias:	High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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