Fig. 10
Plot of 1D non-LTE oxygen abundances in the Galactic disc, as presented by Korotin et al. (2014). Abundances that are based on the analysis of spectra taken at all phases and at optimal phases 0.3 < ϕph < 0.8 are shown as light blue dots and red circles, respectively. Linear fits for these two cases including 1σ uncertainties are presented in red and blue lines.
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