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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Advances in Astronomy

fig14

Figure 14

Figure 14: 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 14 | 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 