Dynamical maps of δψ_i in the osculating (a, e)-plane for a Trojan pair of equal masses, initially placed in the ACR configuration. Initial conditions for the angles are the same as in Fig. 13. Blue islands correspond to libration of ψ ₁ (left panel) or ψ₂ (right panel). Gray regions correspond to circulation of ψ_i, and white regions correspond to unstable orbits (compare to Fig. 7). The upper horizontal axis is the distance in terms of R_Hill.