A stochastic Monte Carlo approach to model real star cluster evolution - II. Self-consistent models and primordial binaries

Monthly Notices of the Royal Astronomical Society

Volumn 317, Issue 3, 2000, Pages 581-606

  Giersz, M ^a,b   Spurzem, R ^b,c  

^a NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^b ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^c UNIVERSITY OF TÜBINGEN   (Germany)

Author keywords

Binaries: general; Celestial mechanics, stellar dynamics; Globular clusters: general; Methods: numerical

Indexed keywords

MONTE CARLO METHODS; NUMERICAL METHODS; STARS; STOCHASTIC MODELS; STOCHASTIC SYSTEMS;

BINARIES:GENERAL; CELESTIAL MECHANIC, STELLAR DYNAMIC; CELESTIAL MECHANICS; GLOBULAR CLUSTERS:GENERAL; MASS STARS; METHOD: NUMERICAL; POINT MASS; STAR CLUSTERS; STELLAR DYNAMICS; STOCHASTICS;

ASTROPHYSICS;

EID: 0000353123     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03727.x     Document Type: Article

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