
doi: 10.1007/bf00641560
Three bodies \(M_ 1\), \(M_ 2\) and M with masses \(m_ 1\), \(m_ 2\) and \(m=0\), and charges \(q_ 1\), \(q_ 2\), \(q=0\) revolve around the centre of mass of the first two in circular orbits attracting (or repulsing) each other according to the Newtonian and Coulombian inverse square law. According to the authors this paper is a generalization of the classical restricted circular three-body problem. A discussion on existence and location of the collinear and equilateral triangle configurations of these bodies is given.
equilateral triangle configurations, Coulombian inverse square law, Three-body problems, existence, circular orbits, generalization of the classical restricted circular three-body problem, Lagrange's equations, location
equilateral triangle configurations, Coulombian inverse square law, Three-body problems, existence, circular orbits, generalization of the classical restricted circular three-body problem, Lagrange's equations, location
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