Fig. 9.

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Comparison of an early spectrum of SN 2018ivc (+10 d) with those at similar epochs of SNe IIn 1996al and 1998S, SNe IIb 1993J and 2011fu, SN IIL 2007fz. The true spectral appearance of SN 2018ivc in the first days is hidden by the effects of interaction. H and He transitions are marked by the continuous and dashed vertical lines, respectively.
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