Hiramatsu, Daichi; Howell, D. Andrew; Van Dyk, Schuyler D.; Goldberg, Jared A.; Maeda, Keiichi; Moriya, Takashi J.; Tominaga, Nozomu; Nomoto, Ken'ichi; Hosseinzadeh, Griffin; Arcavi, Iair; McCully, Curtis; Burke, Jamison; Bostroem, K. Azalee; Valenti, Stefano; Dong, Yize; Brown, Peter J.; Andrews, Jennifer E.; Bilinski, Christopher; Williams, G. Grant; Smith, Paul S.; Smith, Nathan; Sand, David J.; Anand, Gagandeep S.; Xu, Chengyuan; Filippenko, Alexei V.; Bersten, Melina C.; Folatelli, Gastón; Kelly, Patrick L.; Noguchi, Toshihide; Itagaki, Koichi
(2021)
In the transitional mass range (~8-10 solar masses) between white dwarf formation and iron core-collapse supernovae, stars are expected to produce an electron-capture supernova. Theoretically, these progenitors are thought ...