Fig. 6.
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Impact of the dust mass on the spectral properties of the SN IIn model at 300 d. When included, the dust was placed within the dense shell at 5000 km s−1 (purple curve in the top panel of Fig. 5). The figure is analogous to Fig. 5 and shows the impact on the ultraviolet and optical spectrum (top) and on the Hα profile (bottom).
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