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

fig11

Figure 11

Figure 11: 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 11 | 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 