A stochastic Monte Carlo approach to modelling real star cluster evolution - III. Direct integration of three- and four-body interactions

Monthly Notices of the Royal Astronomical Society

Volumn 343, Issue 3, 2003, Pages 781-795

  Giersz, M ^a   Spurzem, R ^b  

^a NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^b ASTRONOMISCHES RECHEN INSTITUT   (Germany)

Author keywords

Binaries: General; Galaxies: star clusters; Methods: numerical; Stellar dynamics

Indexed keywords

ASTROPHYSICS; BINDING ENERGY; GALAXIES; GAS DYNAMICS; MONTE CARLO METHODS; NUMERICAL METHODS; STARS; STOCHASTIC SYSTEMS;

BINARIES:GENERAL; DIRECT INTEGRATION; GALAXIES: STAR CLUSTERS; METHOD: NUMERICAL; MONTE CARLO APPROACH; STAR CLUSTERS; STELLAR DYNAMICS; STOCHASTICS; SYMMETRICS; THREE BODY;

MERGING;

EID: 0142055139     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06717.x     Document Type: Article

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