Fig. 24.
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Left: comparison of the observations of SN 2011dh at 202 d with the He-star explosion model he4p0 at 200 d with a uniform volume filling factor of 50%. Right: same as left, but now using the he5p0 model but scaled down in Ekin and 56Ni mass, and excluding bound-bound transitions from Ni II. Model and observation are normalized at 7000 Å.
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