Evolution of accretion rates, migration, and eccentricities for the models with planetary accretion.Then panels show from top to bottom: the semi-major axis of both planets, a_in/out, the eccentricity of the inner planet and that of the outer planet, e_in/out, planetary mass accretion rate onto the inner and outer planet, Ṁ_in/out, and the mass accretion rate onto the star smoothed with a moving average of length 1.185 kyr, Ṁ_*. The vertical dashed lines indicate events of interest and are referred to in Sect. 3.5. Model A0.0 is an alias for model M9-3.