The collinear libration points in the photogravitational three-body problem

Details The collinear libration points in the photogravitational three-body problem The collinear libration points in the photogravitational three-body problem

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..432k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, July-Aug. 1983, p. 432-435) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, July-

Astronomy and Astrophysics

Astronomy

3

Binary Stars, Celestial Mechanics, Libration, Radiation Pressure, Stellar Motions, Three Body Problem, Collinearity, Gravitational Fields, Systems Stability

Scientific paper

In the restricted circular photogravitational three-body problem, where
a particle moves in the field of two gravitating, radiating mass points,
a three-parameter family of collinear libration points exists. Unlike
the case in the classical problem, there is a domain of parameter space
in which the positions of relative equilibrium are stable.

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