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Fig. 2
Temperature (left) and density (right) profiles of the models of Fig. 1 at the current Uranus age. For comparison, we show the Uranus model H-1 by Helled et al. (2011) and models N-1 and N-2 of Nettelmann et al. (2013). The kinks in the profiles are caused by the non-adiabatic heat transport.
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