Fig. 21
a) and b): the V-brightness of the star from Eq. (17) as deduced by an observer in units of the true maximum stellar brightness. The true stellar brightness is given by the solid line. The models differ in size and, for SN4 also in the scattering properties of the dust. SN4 is otherwise identical to SN1. c) The color excess EB − V(t) for SN4.
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