Non-symmetric doubly-asymptotic orbits at the outer collinear equilibrium pointL 3

In the framework of the solar system case (with only the larger primary radiating) of the photogravitational restricted three-body problem we compute and present some non-symmetric asymptotic orbits connecting the outer collinear equilibrium pointL ₃ with the neighbourhood of one of the triangular equilibrium pointsL _{4, 5}. Such orbits have not been found previously in the restricted problem.