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Sharma, R.K. and Rao, P.S. (1975) Collinear Equilibria and Their Characteristics Exponents in the Restricted Three-Body Problem When the Primaries Are Oblate Spheroids. Celestial Mechanics, 12, 189-201.
https://doi.org/10.1007/BF01230211

has been cited by the following article:

• TITLE: Halo Orbits in the Photo-Gravitational Restricted Three-Body Problem

  AUTHORS: Saurav Ghotekar, Ram Krishan Sharma

  KEYWORDS: Halo Orbits, Circular Restricted Three-Body Problem, Lagrangian Points, Radiation Pressure, Lindstedt-Poincare Method

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.9 No.3, September 5, 2019

  ABSTRACT: We study halo orbits in the circular restricted three-body problem (CRTBP) with both the primaries as the sources of radiation. The positioning of the triangular equilibrium points is discussed in a rotating coordinate system.