Fig. A.1.
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Comparison between the abundance of two identical tracers of oxygen, one of which (vertical axis) includes an initial floor of 2 × 10−5 to promote gas cooling at early times. The figure includes data from three simulations with different seed for random number generation but the same model; yields from LC18, 150 km s−1 for massive stars and tIa = 100 Myr).
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