Fig. 17
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Evolution of the (fractional) net collisional cooling in the nebular phase for the Fe lines (yellow) and the [O i] 6300, 6364 Å (blue) and [Ca ii] 7291, 7323 Å (red) lines in the core (υ = 2900 km s−1) for the macroscopically mixed standard model (circles and solid lines) and the microscopically mixed model (crosses and dashed lines).
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