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

<table>Combined graph for Figures <a href="../fig5/">5</a>, <a href="../fig6/">6</a>, and <a href="../fig7/">7</a>.</table>

Advances in Astronomy

fig13

Figure 13

Figure 13: 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 13 | 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 