2018
DOI: 10.1016/j.amc.2017.11.052
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Periodic solutions around the collinear equilibrium points in the perturbed restricted three-body problem with triaxial and radiating primaries for binary HD 191408, Kruger 60 and HD 155876 systems

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Cited by 10 publications
(19 citation statements)
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“…Assuming that the coordinate of the third particle is (x, y, z), the two primaries are located at (µ, 0, 0) and (µ − 1, 0, 0), respectively. According to Singh et al [17] and Jain et al [10], the equations of motion of the third particle are…”
Section: Dynamical Equationsmentioning
confidence: 99%
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“…Assuming that the coordinate of the third particle is (x, y, z), the two primaries are located at (µ, 0, 0) and (µ − 1, 0, 0), respectively. According to Singh et al [17] and Jain et al [10], the equations of motion of the third particle are…”
Section: Dynamical Equationsmentioning
confidence: 99%
“…In the plane, the motion equations of the third particle are (see [17] When C = 3, the zero-velocity surface of the third particle is shown in Figure 6. The third particle can only skim over two primaries under the action of gravity but cannot pass through the forbidden area around them.…”
Section: Expansion Of the 2d Equations Of Motionmentioning
confidence: 99%
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