Fig. 9

Influence of varied post formation luminosity (Lpf) on the intrinsic luminosity and temperature for four different masses. The colour code is given in the left panel, the line style is given in the right panel. All cooling curves are calculated with a cloud-free atmosphere with solar metallicity in the petitCODE grid. Solid lines show the evolution with the nominal Lpf of Table 2. Dashed lines show the evolution with a ten times bigger Lpf (hot scenario). Dash-dotted lines show the evolution with a ten times fainter Lpf (cold scenario).
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