Carbon Detonation Supernova
Oct. 5, 2024
Simulations uncover why supernova explosions of some white dwarfs produce so much manganese and nickel | Kavli IPMU-カブリ数物連携宇宙研究機構 Simulation of a SUPERNOVA DETONATION in pure carbon isotope (C-12) - YouTube Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications | Science Carbon Detonation Supernova
![PDF] Double-detonation supernovae of sub-Chandrasekhar mass white dwarfs | Semantic…](https://d3i71xaburhd42.cloudfront.net/18b6c173787bf40012d82c556c0ded1bc153cb52/6-Figure3-1.png){kind=link}
![PDF] A subgrid-scale model for deflagration-to-detonation transitions in type Ia su…](https://d3i71xaburhd42.cloudfront.net/80b4a59ee06e019eb7a82ea17c61c93e3b9f12b6/5-Figure1-1.png){kind=link}
![PDF] Double-detonation supernovae of sub-Chandrasekhar mass white dwarfs | Semantic…](https://d3i71xaburhd42.cloudfront.net/18b6c173787bf40012d82c556c0ded1bc153cb52/4-Figure1-1.png){kind=link}
.jpg){kind=link}
.jpg){kind=link}
![PDF] DOUBLE-DETONATION SUB-CHANDRASEKHAR SUPERNOVAE: SYNTHETIC OBSERVABLES FOR MINI…](https://d3i71xaburhd42.cloudfront.net/cb3a2f706e7891cd1b4a88fa5c0c412e7fcb2311/3-Figure1-1.png){kind=link}
