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Fig. C.3

image

Reduction of the planetesimal impact heating in case of no sinking relative to the sinking case (Eq. (C.20)). The dots show Lpla,nosink/Lpla,sink as a function of mass for synthetic planets with Menv ≤ 2Mcore in the CD777 population at 2 Myr. The color code shows the envelope mass fraction Menv/M. Near crossover, the heating efficiency is reduced by typically a factor 3 with a spread of 2.5–8.

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