Fig. 1
Reference angles represented for the circular co-orbital system with respect to an inertial frame (x,y). m0 is the mass of the central star, m1 and m2 the masses of the co-orbitals. ri is the distance of the co-orbital i to the central star, and λi its true longitude. Following Eq. (3) one can write λi as a function of λ0, ζ, and of the mass ratio δ.
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