A new method to create initially mass segregated star clusters in virial equilibrium

Monthly Notices of the Royal Astronomical Society

Volumn 385, Issue 3, 2008, Pages 1673-1680

  Subr L ^a,b,c   Kroupa, P ^a   Baumgardt, H ^a  

^a UNIVERSITY OF BONN   (Germany)

^b CHARLES UNIVERSITY   (Czech Republic)

^c ASTRONOMICAL INSTITUTE   (Czech Republic)

Author keywords

Methods: N body simulations; Methods: statistical; Stellar dynamics

Indexed keywords

STARS;

DYNAMICAL EVOLUTION; INTERPARTICLE POTENTIAL; MASS SEGREGATION; METHODS:N-BODY SIMULATIONS; METHODS:STATISTICAL; PARAMETER GENERALIZATION; SINGLE PARAMETER; STAR CLUSTERS; STELLAR DYNAMICS; VIRIAL EQUILIBRIUM;

GRAVITATION;

EID: 41649107670     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.12993.x     Document Type: Article

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