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The problem of restricted three bodies is considered. The treatment is carried out within the framework of the post-Newtonian approximation. The primaries also are assumed to be radiant sources. The locations of the collinear points are computed. Series forms of these locations are obtained as new results. A Mathematica program is constructed so as to draw the locations of collinear points versus the whole range of the mass ratio μ taking into account the photo-gravitational effects and/or the relativistic corrections. Analyses of these figures are addressed

Analytical and Semianalytical Treatment of the Collinear Points in the Photogravitational Relativistic RTBP