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A stochastic Monte Carlo approach to modelling real star cluster evolution – III. Direct integration of three- and four-body interactions
Authors:M. Giersz   R. Spurzem
Affiliation:Nicolaus Copernicus;Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland Astronomisches Rechen-Institut, Mönchhofstraße 12–14, D-69120 Heidelberg, Germany
Abstract:
Keywords:stellar dynamics    methods: numerical    binaries: general    galaxies: star clusters
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