Fig. 4

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Non-LTE mechanism for a model at roughly solar parameters (Teff = 5750 K, log 𝑔 = 4.5 cm s−2, [Fe/H]= 0) in the left panels and for a hotter star (Teff = 7000 K, log 𝑔 = 4.0 cm s−2, [Fe/H]= 0) showing larger departures from LTE in the right panels. In each case, the upper panel shows the run of the departure coefficient b_ with the logarithm of the optical depth at 500 nm, log τ500. The second panel shows the ratio R†/R. The third panel shows the photodetachment rate per H− ion R and effective collisional rate per H− ion r. The lowest panel shows the temperature T. In each case, models with standard convection for MARCS models (mixing length parameter α = 1.5, thinner blue lines) and without convection (α = 0, thicker orange lines) are shown.
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