Fig. 6
Density profile of the MS_110 model for different times after the SN explosion. The black solid line corresponds to the initial density profile of the star at the moment of the explosion. All black dashed lines froma ◯toe ◯show the radial density distribution of the star (0.4,0.8···2.0) × 104 s after the impact in time intervals of 4000 s.
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