Stellar escapes from isolated clusters. IV - Numerical methods

Details Stellar escapes from isolated clusters. IV - Numerical methods Stellar escapes from isolated clusters. IV - Numerical methods

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979poast..27..107k&link_type=abstract

Postepy Astronomii, vol. 27, Apr.-June 1979, p. 107-111. In Polish.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Star Clusters, Stellar Motions, Stellar Systems, Equations Of Motion, Escape, Gravitational Effects, Monte Carlo Method, Numerical Integration, Rates (Per Time)

Scientific paper

The three numerical methods proposed in the present paper for
calculating the evolution of stellar systems are a Monte Carlo
technique, a gasdynamic method, and a method based on the integration of
the equations of motion. The stellar escape velocities calculated by
these methods are shown to correlate well with analytical results.

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