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SN 2023ixf in the Pinwheel Galaxy M101: From Shock Breakout to the Nebular Phase

We present photometric and spectroscopic observations of supernova SN 2023ixf covering from day 1 to 442 days after explosion. SN 2023ixf reached a peak V -band absolute magnitude of −18.2 ± 0.07, and light curves show that it has a relatively short “plateau” phase (∼72 days), and can be classified...

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Kaydedildi:
Asıl Yazarlar: WeiKang Zheng, Luc Dessart, Alexei V. Filippenko, Yi Yang, Thomas G. Brink, Thomas de Jaeger, Sergiy S. Vasylyev, Schuyler D. Van Dyk, Kishore C. Patra, Wynn V. Jacobson-Galán, Gabrielle E. Stewart, Efrain Alvarado III, Veda Arikatla, Pallas Beddow, Andreas Betz, Emma Born, Kate Bostow, Adam J. Burgasser, Osmin Caceres, Evan M. Carrasco, Elma Chuang, Asia DeGraw, Elinor L. Gates, Eli Gendreau-Distler, Cooper Jacobus, Connor Jennings, Preethi R. Karpoor, Paul Lynam, Ann Mina, Katherine Mora, Neil Pichay, Jyotsna Ravi, Jon Rees, R. Michael Rich, Sophia Risin, Nathan R. Sandford, Alessandro Savino, Emma Softich, Christopher A. Theissen, Edgar P. Vidal, William Wu, Yoomee Zeng
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2025-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Supernovae
Type II supernovae
Online Erişim:https://doi.org/10.3847/1538-4357/ade0bf
Etiketler: Etiketle
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