Fig. 7

The combined night and day side cooling as a function of the surface gravity and core entropy. It is expressed as the intrinsic effective temperature in K. Left: the effect of the Pn parameter. The models are calculated for three different values of Pn = 0.1,0.3,0.5. The total core heat loss decreases with increasing Pn. Right: the effect of the depth of the heat redistribution. The models are calculated for three different values of the day side Rosseland optical depth of the bottom of the heat redistribution region τross = 1,3,9. Total heat loss decreases with increasing optical depth. See the text for a more detailed discussion.
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