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SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material

Fuente: arXiv

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Bibliographic Details
Main Authors:	Peng, Z. -H., Benetti, S., Cai, Y. -Z., Pastorello, A., Valerin, G., Reguitti, A., Fiore, A., Fang, Q. -L., Wang, Z. -Y., Berton, M., Borsato, L., Cappellaro, E., Congiu, E., Elias-Rosa, N., Granata, V., Isern, J., La Mura, G., Ochner, P., Raddi, R., Terreran, G., Tomasella, L., Turatto, M., Yan, S. -Y., Pei, S. -P., Wu, C. -Y., Zha, S., Wang, X. -F., Wang, B., Pan, Y.
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2511.12929