Fig. 6.
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Difference in Teff, log g, [Fe/H], ξmicro, [C/Fe], and [N/Fe] as a function of the difference in [O/Fe] resulting from the changed population assumption from thin to thick disk and vice versa for the 44 solar neighborhood M giants. Circles with positive δ[O/Fe] values represent thin-disk stars that were assumed to be thick-disk stars for this exercise.
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