Fig. 1
Atmospheric temperature as a function of the logarithm of the Rosseland optical depth for DA models with effective temperatures of 8000 (bottom) and 12 000 K (top). We show the standard 1D structures (solid black line) from Tremblay et al. (2011a), recomputed with a slightly higher numerical precision, and the improved 1D LHD structures (dashed blue line) described in the text.
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