Fig. 11.
Spectral comparison between SN 2017cbv (black) and our models. From left to right panels show spectra at 1.5, 3.5, and 18.5 days after explosion. Each spectrum is offset vertically for clarity, with a dashed line showing the zero-point for each offset. The region showing strong flux suppression at maximum light in our shell models is given by a shaded grey region.
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