Fig. 7
Results for the 19 M⊙ clumpy model: Top-left: SiO mass as a function of post-explosion time. Observational data for several supernovae are given as symbols. Top-right: dust mass as a function of post-explosion time and dust type. Bottom-left: grain size distributions of the various dust components at day 2000. Bottom-right: mass distributions of the various dust components at day 2000.
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