Remarks on the photogravitational restricted three-body problem

Details Remarks on the photogravitational restricted three-body problem Remarks on the photogravitational restricted three-body problem

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.201..281t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 201, no. 2, p. 281-285.

Statistics

Computation

3

Binary Stars, Computational Astrophysics, Gravitational Effects, Lagrangian Equilibrium Points, Three Body Problem, Radiation Pressure, Stellar Systems, Two Body Problem

Scientific paper

The effects of the radiation pressure in the restricted three-body problem are considered and the existence of the 'out-of-plane' equilibrium points is analyzed. It is found that within the framework of the stellar stability, the five Lagrangian points are the only equilibrium points, at least as far as the force of the radiation pressure is taken into account.

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