Fig. C.2.
Variation of κ[CII](H0) calculated for six combinations of T and n as a function of metallicity as traced by the oxygen abundance. The vertical yellow line shows the assumed value for solar metallicity (12 + log(O/H) = 8.65; Simón-Díaz & Stasińska 2011). The right ordinate shows in red the dependence on the carbon abundance [C/H] as a function of metallicity from the MAPPINGS code (Nicholls et al. 2017).
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