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Fig. 15.
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Comparison of SN 2021adxl to the Type IIn SN 2010jl (Fransson et al. 2014), as well as the transitional Type Ic-BL/IIn SN 2017ens (Chen et al. 2018). The insets highlight the wavelength range around known coronal emission lines. Each inset has been normalized to the peak of each respective emission line.
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