no code implementations • 8 Feb 2021 • A. A. Nikiforova, P. V. Baklanov, S. I. Blinnikov, D. A. Blinov, T. S. Grishina, Yu. V. Troitskaya, D. A. Morozova, E. N. Kopatskaya, E. G. Larionova, I. S. Troitsky
The model progenitor mass $M=25 M_\odot$ significantly exceeds the upper limit mass $M=17 M_\odot$, obtained from analysis the pre-SNe observations.
High Energy Astrophysical Phenomena
