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Fig. 10


Si  iiλ6355 expansion velocity evolution of SN 2010ev derived from the minimum of the absorption line, compared with other SNe: SN 2009Y, SN2006X (Wang et al. 2008; Yamanaka et al. 2009), SN2005cf (Pastorello et al. 2007), SN2004dt (Altavilla et al. 2007), SN2003du (Stanishev et al. 2007), SN2002dj (Pignata et al. 2008), SN2002bo (Benetti et al. 2004), SN1994D (Patat et al. 1996), H07 template, and B15 model.

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