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Fig. 3


Best-fit hydrodynamic model. Panel a): the bolometric light curve of the best-fit model (solid line) overplotted on the bolometric data of SN 2012A (crosses) evaluated from the UBVRIJHK magnitudes reported by Tomasella et al. (2013). Panel b): the calculated photospheric velocity (solid line) compared to the photospheric velocity derived from the Hα and Hβ lines (open circles) (Sect. 2) and from the He i 5876 Å line (filled circles, Tomasella et al. 2013). Panels c) and d): the calculated B and R light curves (solid line) compared to the observations of SN 2012A (crosses) obtained by Tomasella et al. Two open circles are the SN detection in R band (Moore et al., 2012).

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