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Fig. 11

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[C/H] for the simulation HKB-fid as a function of time for Jupiter and Saturn. The uncertainties are shown by the extent of the filled-in areas and are due to the uncertainties over the respective atmospheric mass in which the CO can mix (i.e. between a diluted 60 M diffuse core for both planets and a 20, 30 M solid core for Saturn and Jupiter, respectively).

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