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A Robust Light-curve Diagnostic for Electron-capture Supernovae and Low-mass Fe-core-collapse Supernovae

Core-collapse supernovae (CCSNe) are the terminal explosions of massive stars. While most massive stars explode as iron-core-collapse supernovae (FeCCSNe), slightly less massive stars explode as electron-capture supernovae (ECSNe), shaping the low-mass end of CCSNe. ECSNe were proposed ∼40 yr ago an...

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Principais autores: Masato Sato, Nozomu Tominaga, Sergei I. Blinnikov, Marat Sh. Potashov, Takashi J. Moriya, Daichi Hiramatsu
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/ad50cb
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