Abstract
The effect of the radiation pressure on the periodic motion of a small particle around one ‘primary’ body of the restricted photogravitational three-body problem is examined. Simple periodic orbits are used to determine the maximum size of the accretion disk in close binary systems.
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Niedzielska, Z. Periodic Orbits and Accretion Disks. Celestial Mechanics and Dynamical Astronomy 67, 205–213 (1997). https://doi.org/10.1023/A:1008209210002
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DOI: https://doi.org/10.1023/A:1008209210002