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Fig. 1

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Mean temperature structure as a function of Rosseland optical depth of the CO5BOLD model used in this work (Teff  = 5850 K, log g = 4.0,  [Fe/H ]  =  −4.0; thick [blue] line), and of the 3D model used in Caffau et al. (2011c) (5850/4.0/ − 3.0; thin [red] line). For each model, the mean temperature is obtained by averaging the temperature as over iso-τRoss surfaces of 20 selected snapshots. Shaded areas bounded by dashed lines indicate the  ± 1σ range of deviations. Small open symbols outline the temperature stratification of the 1DLHD model with  [Fe/H ]  =  −4.

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