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Fig. 8


Dependence of the bolometric light curve and the hydrogen mixing on the chemical composition of the hydrogen-rich envelope for the late-time 1D N20 models with the representative radioactive 56Ni mass from Table 2. Panel a): bolometric light curves of models N20-P (black line) and N20-C (red line). Panel b): mass fraction of hydrogen as function of velocity in models N20-P (black line) and N20-C (red line). Panels c) and d): mass fractions as functions of velocity in models N20-P and N20-C, respectively. The red line is the mass fraction of radioactive 56Ni, and the magenta line represents iron-group elements except for 56Ni (see also Fig. 2). All profiles of the mass fractions are given at t = 50 days.

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