Fig. 13.
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Relation between the radius and mass of the envelope for the SNe IIb progenitor models (blue dots) from Ouchi & Maeda (2017). The black line represents the analytical relation derived by Ouchi & Maeda (2017), which captures the properties of the numerical evolution models. The parameters derived for SN 2017ckj are indicated by the red star. This figure is modified from Gangopadhyay et al. (2023).
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