Browse Journals

[1] K. B. Bhatnagar and J. M. Chawla, Stability of triangular Lagrangian points in the restricted three-body problem, Celestial Mechanics 19(1), 1-7 (1979).

[2] NASA, James Webb Space Telescope: Lagrange point 2 (L2) Retrieved from https://www.nasa.gov (2021).

[3] V. V. Radzievskii, The effect of radiation pressure on the motion of small bodies in the solar system, AstronomicheskiiZhurnal, 27, 250-253 (1950).

[4] A. E. Roy, Orbital Motion (4th Ed.). CRC Press, 2005.

[5] J. Singh and A. Taura, The influence of radiation pressure on the location and stability of Lagrangian points, Astrophysics and Space Science 354(2) (2014), 449-460.

[6] V. Szebehely, Theory of orbits: The Restricted Three-Body Problem, Academic Press, 1967.

[7] A. Sharma and R. Sharma, Effect of Radiation Pressure on the Collinear Lagrangian Points in the Photogravitational Restricted Three-Body Problem, Astrophysics and Space Science 368(2) (2023).

[8] M. Patel and R. K. Upadhyay, Stability of Lagrangian Points in the Presence of Radiation and Oblateness Effects, New Astronomy 101, 102056 (2023).

[9] R. Kumar, S. Singh and A. Mishra, Radiation Pressure and Lagrangian Point Dynamics in Celestial Systems. Advances in Space Research 72(6) (2023), 2031-2040.

[10] M. Ali and J. Singh, Photogravitational effects on the triangular equilibrium points under modified Newtonian dynamics, Astrophysics and Space Science 368(5) (2023).

[11] A. Das and S. Mondal, Influence of Radiation Pressure on the Non-Planar Equilibrium Points in the Restricted Three-Body Problem, Celestial Mechanics and Dynamical Astronomy 136(3) (2024).