A statistical theory of the disruption of three-body systems. II - High angular momentum

Details A statistical theory of the disruption of three-body systems. II - High angular momentum A statistical theory of the disruption of three-body systems. II - High angular momentum

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177..583m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Dec. 1976, p. 583-594.

Astronomy and Astrophysics

Astronomy

23

Angular Momentum, Statistical Analysis, Ternary Systems, Three Body Problem, Conservation Equations, Disrupting, Escape Velocity, Phase-Space Integral, Velocity Distribution

Scientific paper

The statistical theory of the disruption of three-body self-gravitating
systems is refined by allowing for both energy and angular momentum
conservation in the phase-space description. The resulting distribution
of the parameters of the remnant binary and the velocity distribution of
the escaping particle are in good agreement with numerical experiments.

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