Existence of Resonance Stability of Triangular Equilibrium Points in Circular Case of  the Planar Elliptical Restricted Three-Body Problem  under the Oblate and Radiating Primaries around the Binary System

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q-14 98 -31 149.5t-50 51.5q-49 0 -94 -70t-45 -164q0 -55 15.5 -86t40.5 -31q70 0 164 150z" id="x1D6FC"></path></g>
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Advances in Astronomy

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Figure 3

Figure 3: Existence of Resonance Stability of Triangular Equilibrium Points in Circular Case of  the Planar Elliptical Restricted Three-Body Problem  under the Oblate and Radiating Primaries around the Binary System 

Figure 3 | Existence of Resonance Stability of Triangular Equilibrium Points in Circular Case of  the Planar Elliptical Restricted Three-Body Problem  under the Oblate and Radiating Primaries around the Binary System 