Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs

Open Access

Fig. 7.

Velocity versus “spherical” mass (i.e., ∫4πr²ρdr) obtained with the radiation-hydrodynamics code V1Dfor the b = 0.15 case at multiple times up to 1 d (top) and the full model set at 1 d (bottom). A velocity hole is observed in the unbound debris below ∼3000 km s⁻¹ due to fallback of material.

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