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Fig. 5


Top row: Comparison of the density and temperature profiles at 1.2 d for the H-rich models. The more massive and extended is the low-mass H-rich envelope, the greater is the outer ejecta temperature. Bottom row: Composition profiles for models H_R61 and H_R601 at 1.2ḋ (see also Fig. B.1). The dashed line corresponds to 56Ni. This time corresponds to the time of remapping into CMFGEN.

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