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Fig. 9


Bolometric light curves of model B15-2 with the mass scaled to fit the observed luminosity in the radioactive tail, (see Table 4) (blue line), the mass of radioactive 56Ni produced directly by our reaction network, (magenta line), and the aggregate mass of directly produced 56Ni and tracer nucleus, (green line) (see Table 2) for the late-time 1D simulations compared with the observations of SN 1987A obtained by Catchpole et al. (1987, 1988) (open circles) and Hamuy et al. (1988) (open triangles).

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