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Normalisation at the Triangular Equilibria in The Doubly Photogravitational Restricted Problem
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In order to study the stability in the sense of Lyapunov of the triangular equilibria L4 and L5 in the circular restricted problem of three bodies when both finite masses are radiating, the normalization of the second order terms of the Hamiltonians has been done. Special attention is paid to the problem of determining the curves in the parameter plane along which the system presents resonances of the type (1:1), (1:2) and (1:3).
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