The study of a stellar system containing a massive central binary using a numerical experiment

Details The study of a stellar system containing a massive central binary using a numerical experiment The study of a stellar system containing a massive central binary using a numerical experiment

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...67b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, May-June 1987, p. 67-71. In Russian.

Computer Science

Binary Stars, Celestial Mechanics, Particle Trajectories, Stellar Mass, Stellar Systems, Three Body Problem, Radial Velocity, Temporal Distribution

Scientific paper

A method is proposed for the study of systems consisting of massive bodies moving among lighter particles. The method involves tracking of the trajectories of a comparatively small number of bodies for a long period of time and determining various characteristics by means of averaging. The interaction between the massive binary and the surrounding system is investigated by solving the restricted circular three-body problem. It is found that, in the present model, the lighter particles accumulate in the vicinity of the binary.

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