Sharma, R.K. and Rao, P.V.S. (1976) Stationary Solutions and Their Characteristic Exponents in the Restricted ThreeBody Problem When the More Massive Primary Is an Oblate Spheroid. Celestial Mechanics, 13, 137-149. http://dx.doi.org/10.1007/BF01232721

has been cited by the following article:

• TITLE: The Collinear Libration Points in the Elliptic R3BP with a Triaxial Primary and an Oblate Secondary

  AUTHORS: Jagadish Singh, Aishetu Umar

  KEYWORDS: Celestial Mechanics, ER3BP, Triaxiality, Oblateness, Collinear Points

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.4 No.2, June 10, 2014

  ABSTRACT: This paper examines the motion of a dust grain around a triaxial primary and an oblate companion orbiting each other in elliptic orbits about their common barycenter in the neighborhood of collinear libration points. The positions and stability of these points are found to be affected by the triaxiality and oblateness of the primaries, and by the semi-major axis and eccentricity of their orbits. The stability behavior of the collinear points however remains unchanged; they are unstable in the Lyapunov sense.