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SN 2023ixf in M101: physical parameters from bolometric light curve modeling

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Vinko, J., Bodola, Zs. R., Godeny, A., Csak, Sz. F., Konyves-Toth, R., Nagy, A. P., Szalai, T., Banhidi, D., Biro, I. B., Bodi, A., Bora, Zs., Csanyi, I., Cseh, B., Hegedus, T., Horti-David, A., Joo, A. P., Kalup, Cs., Kriskovics, L., Mochnacs, E., Pal, A., Regaly, Zs., Seli, B., Sodor, A., Szabo, N. O., Szakats, R., Szekely, P., Varga, V., Vida, K.
Formato:	Preprint
Publicado:	2025
Materias:	High Energy Astrophysical Phenomena 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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