Fig. 20

Results of the N-body simulation with ,
,
, and Mi = 10,
Mo = 20 M⊕
are over-plotted on those of 2p20 DZ model. The dark and light colours refer to the
N-body and hydrodynamical simulation. To facilitate the comparison, we shifted the time axis for the hydrodynamical simulation such that the t = 0 orbit corresponds to the time at which the planets are just outside of 4:3 resonance.
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