The binaries and triple systems in an irregular field

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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