Fig. 5.
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Impact of the dust location on the spectral properties of the SN IIn model at 300 d. We show various choices for the dust spatial distribution (top) and the corresponding predictions for the resulting optical spectrum (middle) and the Hα profile (bottom). The dust is made of 0.1μm silicate grains and the total dust mass is 10−4 M⊙. [See Sect. 5 for discussion.]
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