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Fig. 2

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Model LMIN. Selected evolutionary stages of the SN interaction with the ’thinnest’ bipolar lobes structure calculated by the RHD code. The four columns show the snapshots at times t = 0, 240, 480, and 730 days. The individual rows show four different quantities: from top to bottom it is density ρ, velocity magnitude v, temperature T, and radiative energy density Er. The animated version of this image is available online.

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