Fig. 8
Illustration of impact of model parameters θ6,7 = xout,fcorona, the mass loading or outflow fraction and the corona mass factor on the ISM metallicity. The resulting metallicity of ISM gas (upper panel) and corona gas (lower panel) is shown over time assuming the default yields. The results for 
are compared with ± 2σprior deviations and our observational constraints.
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