SN 2023ixf in M101: Physical Parameters from Bolometric Light Curve Modeling

Abstract We present new photometric observations of the core-collapse supernova SN 2023ixf occurred in M101, taken with the RC 80 and BRC80 robotic telescopes in Hungary. The initial nickel mass from the late-phase bolometric light curve extending up to 400 days after explosion, is inferred as M Ni = 0.046 ± 0.007 M ⊙ . The comparison of the bolometric light curve with models from hydrodynamical simulations as well as semi-analytic radiative diffusion codes reveals a relatively low-mass ejecta of M ej ≲ 9 M ⊙ , contrary to SN 2017eaw, another H-rich core-collapse event, which had M ej ≳ 15 M ⊙ .

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Publication Details

Journal
The Astrophysical Journal
Published
2025-10-23
DOI
https://doi.org/10.3847/1538-4357/ae0614
Citations
1
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
1.15
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article

SN 2023ixf in M101: Physical Parameters from Bolometric Light Curve Modeling

Zsófia Bora, I Bíró, B. Cseh, Á. Sódor et al.
1 citations
The Astrophysical Journal
Gamma-ray bursts and supernovae
1.15
article

SN 2023ixf in M101: Physical Parameters from Bolometric Light Curve Modeling

Zsófia Bora, I Bíró, B. Cseh, Á. Sódor, P. Székely, Csilla Kalup, Zsolt Regály, József Vinkó, L. Kriskovics, Réka Könyves-Tóth, István Csányi, B. Seli, Andrea Nagy, Ágoston Horti-Dávid, K. Vida, Tamás Szalai, András Pál, Attila Bódi, Róbert Szakáts, András Péter Joó, Zsofia R. Bodola, D. Bánhidi, Norton Olivér Szabó, V. Varga, Tibor Hegedüs, Erika Mochnács, Ákos Gődény, Szelina Fruzsina Csák
article en
1 citations

Abstract

Abstract We present new photometric observations of the core-collapse supernova SN 2023ixf occurred in M101, taken with the RC 80 and BRC80 robotic telescopes in Hungary. The initial nickel mass from the late-phase bolometric light curve extending up to 400 days after explosion, is inferred as M Ni = 0.046 ± 0.007 M ⊙ . The comparison of the bolometric light curve with models from hydrodynamical simulations as well as semi-analytic radiative diffusion codes reveals a relatively low-mass ejecta of M ej ≲ 9 M ⊙ , contrary to SN 2017eaw, another H-rich core-collapse event, which had M ej ≳ 15 M ⊙ .

The Astrophysical JournalVol. 993(1)
Openalex Percentile: Top 15%
Gamma-ray bursts and supernovae
1.15
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