Late encounter events as source of disks and spiral structures - Forming second generation disks

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Fig. 3

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Column density in the planes perpendicular to the orientation of the angular momentum vector for runs IrrI1_t0, IrrI1_t500, IrrI1_t1000, and IrrI1_t at times (t₀ = 0, t₁ = 4 t_dyn, t₂ = 8 t_dyn, and t₃ = 16 t_dyn.

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