Embedded Files
2D Hydrodynamical models showing type Ia supernova explosions originated from the near-Chandrasekhar mass white dwarf.
A Model with flame transits from deflagration to detonation (DDT)
inset_plot_video.mp4Models with flame fail the transition to detonation.
video_inset_plots.mp4video_inset_plot.mp4Illustration showing the temperature evolution inside the white dwarf. Flame progression from the center of the white dwarf to the surface of the northern hemisphere ejects the highly neutronized material to the interstellar medium (ISM).
3D Hydrodynamical simulations of helium-ignited binary white dwarf mergers.
dens_temp_isocontours_video.mp4dens_temp_isocontours_video_quad_det_model_high_res.mp4Page updated
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