Fig. C.1.

Evolution of the amplitude of libration of the resonant angle ζmax − ζmin (top) and mean eccentricities (bottom) for co-orbitals (m1/m2 = 6) captured in a 4:3 MMR with an outer planet such that m3/m1 = 1 (blue), m3/m1 = 1.6 (purple) and m3/m1 = 2.5 (red). The solid lines show the eccentricity of m2, while the dashed ones show the eccentricity of m1. Both amplitudes of libration and mean eccentricities are taken over a single libration period. These trajectories correspond to 3 cases of the top-right panels of Figs. C.2 and C.3.
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