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Fig. A.2.
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Molecular carbon number density as a function of the Rosseland mean optical depth for DQZ white dwarfs with Teff = 8000 K, log g = 8, log C/He = −5.5, and different Ca/He values (the black line corresponds to log Ca/He = −11.5 and the red line to log Ca/He = −9.5).
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