Fig. 20
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Light-curve models for different spin periods with ejecta masses and magnetic fields derived from the 6O-4-2e39-1e5 and 6O-1.5-1e39-1e6 models, compared with V-band photometric data of SN 2012au from Milisavljevic et al. (2013). The most consistent model has a spin period P0 of 15 ms, and its parameters were derived from the 6O-1.5-1e39-1e6 model.
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