Fig. 15.
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Schematic of the ejecta structure, showing a combination of the 56Ni-rich high-velocity component confined in a narrow solid angle and the slower quasi-spherical ejecta. The black line shows the photosphere at: i) 6 days, when it includes the high-velocity high-velocity component, and ii) at 18 days, when the photosphere recedes in the inner ejecta.
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