Fig. 8
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Mass distributions of Fe-rich ejecta as a function of the velocity component along the LoS (upper panel) and the radial velocity (lower panel) at t ≈ 36 years after core collapse (corresponding to February 2023) for models B18.3 (dashed lines) and B18.3-Dec (solid lines). Red and blue curves represent the results for the southern and northern hemispheres, respectively.
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