no code implementations • 24 Dec 2020 • Takashi Yoshida, Tomoya Takiwaki, Kei Kotake, Koh Takahashi, Ko Nakamura, Hideyuki Umeda
Our 3D results show that turbulent mixing occurs in both of the progenitors with the angle-averaged turbulent Mach number exceeding $\sim$ 0. 1 at the maximum.
Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
