The disintegration of small stellar systems

Details The disintegration of small stellar systems The disintegration of small stellar systems

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1073t&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, July 1984, p. 1073-1075.

Statistics

Applications

Celestial Mechanics, Four Body Problem, Star Clusters, Stellar Motions, Stellar Systems, Three Body Problem, Angular Momentum, Perturbation Theory

Scientific paper

Numerical studies of the disintegration of slightly perturbed equilibrium configurations of three and four bodies reveal that the angular momentum vectors of the final subsystems are substantially randomized for four-body (and greater) systems but are not for three-body systems. The cause of this difference and some possible applications of these findings are discussed.

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