Basic N-body modelling of the evolution of globular clusters - I. Time scaling

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 3, 1998, Pages 794-806

  Aarseth, S J ^a   Heggie, D C ^b  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

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

Indexed keywords

ASTROPHYSICS; NUMERICAL METHODS; STARS;

BODY MODELS; CELESTIAL MECHANIC, STELLAR DYNAMIC; CELESTIAL MECHANICS; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; MASS LOSS; METHOD: NUMERICAL; SCALINGS; STELLAR DYNAMICS; TIME-SCALING;

GRAVITATION;

EID: 0039389330     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01521.x     Document Type: Article

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