Fig. 11
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The growth of the planetary core up to the crossover mass accounting for envelope enrichment caused by pebble evaporation. The blue lines show the case with Ms = 1 M⊙, t0 = 106 yr, αturb = 10−3 and fg = 1. The gray lines show the case without envelope enrichment. Panel a: time evolution of total mass (solid line), envelope mass (dashed line), and core mass (dotted line). Panel b: time evolution of the bulk metallicity of planetary envelope. Panel c: evolution of planetary masses as a function of the total mass. Panel b: evolution of the bulk metallic-ity of planetary envelope vs. the total mass of protoplanet. The vertical dashed lines in Panels c and d are pebble isolation mass.
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