Fig. 18.
Measurements of the pseudo-equivalent width of the Fe II λ5018 line for ASASSN-14jb (black stars), with the correspondent epoch since explosion t0 = 56946.1 ± 3 (MJD). The solid lines show Dessart et al. (2013) models for progenitors with different metallicities and the dashed lines show models with Solar metallicity and different initial radii.
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