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Fig. 10.
Expansion velocities of the Hβ (top), Fe II λ5169 (middle), and Hα (bottom) lines as a function of time after explosion in the plateau phase, measured from the P-cygni profile minima of the Balmer lines Hα, Hβ and the Fe II λ5169 line for ASASSN-14jb (black filled stars) and the Type II SNe comparison sample.
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