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

We present optical photometric and spectroscopic observations of the rapidly declining Type IIL supernova (SN) 2016iog. SN 2016iog reached its peak ∼14 days after explosion, with an absolute magnitude in the V band of −18.64 ± 0.15 mag, followed by a steep decline of 8.85 ± 0.15 mag (100 d)−1 post-p...

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主要な著者:	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.
フォーマット:	Artigo
言語:	Inglês
出版事項:	EDP Sciences 2026-01-01
シリーズ:	Astronomy & Astrophysics
主題:	circumstellar matter stars: mass-loss supernovae: general supernovae: individual: sn 2016iog
オンライン･アクセス:	https://www.aanda.org/articles/aa/full_html/2026/01/aa56330-25/aa56330-25.html
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