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Fig. 3

image

Montage of spectra for the set of WH07 models (blue label) and S16 models (red label) at 350 days after explosion. The wavelength range is limited to the 5600–7500 Å region to reveal the variations in [O I] λλ 6300, 6364, Hα, and [Ca II] λλ 7291, 7323. We note the non-monotonic evolution of these line fluxes with increasing initial mass in the S16 models, in contrast to the results obtained for the WH07 models.

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