States of strong gravitational interaction in the general three-body problem

Details States of strong gravitational interaction in the general three-body problem States of strong gravitational interaction in the general three-body problem

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..152a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Jan.-Feb. 1989, p. 152-160. In Russian.

Astronomy and Astrophysics

Astronomy

9

Celestial Mechanics, Gravitational Effects, Three Body Problem, Computerized Simulation, Evolution (Development), Trajectory Analysis

Scientific paper

The states of the 'triple approach' of bodies at the beginning of the dynamic evolution of systems are studied via computer simulation using the three-body problem with components having equal masses and zero initial velocities. Regions of initial configurations of the triple systems are found in which the actual decay of the system takes place after the first triple approach of the bodies. These regions are situated along the isolines of the ratios of the distances between the components at the initial time.

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