Fig. 13.
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Evolution of the Hα profile in selected spectra of the ILRT AT 2013la (left panel), SN 2018zd (Zhang et al. 2020, middle panel), and the underluminous Type IIP SN 2005cs (Pastorello et al. 2006, 2009, right panel). The Hα lines are shown in the velocity space, with zero velocity (rest wavelength) being marked by a grey dashed line.
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