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Fig. 9


Density evolution of quasi-hydrostatic Mark1R planetary models that fit the observational mass constraints for CoRoT-30 b (top) and CoRoT-31 b (bottom). Blue vertical lines mark the youngest and oldest inferred stellar ages. Red shaded ellipses fit the 1, 3, and 5σ limits for the planetary density at the inferred stellar ages. Full, dashed, and dotted lines mark planet models for high, medium, and low assumptions about the planetesimal accretion rate in the Mark1 ensemble.

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