Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..209a&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 2, Nov. 1989, p. 209-220.
Astronomy and Astrophysics
Astrophysics
5
Binary Stars, Gravitational Collapse, Many Body Problem, Star Clusters, Stellar Evolution, Triple Stars, Digital Simulation, Dynamic Characteristics, Galactic Clusters, Galactic Evolution
Scientific paper
The dynamical evolution of the N-body systems (N = 6) has been studied by numerical simulations. The double and triple subsystems isolated from other bodies have been revealed. The processes of their formation, evolution, and disruption have been followed. At the initial stage of evolution, a common collapse of the system takes place. After that some fast triple approaches of single bodies are possible. At further stages, some physically connected triple subsystems are formed which are disrupted by the intruders or due to their own dynamical unstability. The dissipation mechanisms formulated by van Albada (968) and Aarseth (1973) have been confirmed. At the final stage, double or hierarchical triple systems are formed.
Anosova Zh. P.
Orlov Victor V.
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