The influence of mass-loss from a star cluster on its dynamical friction -I. Clusters without internal evolution

Monthly Notices of the Royal Astronomical Society

Volumn 375, Issue 2, 2007, Pages 604-614

  Fellhauer, M ^a,b   Lin, D N C ^b  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b University of California at Santa Cruz   (United States)

Author keywords

Galaxies: dwarf; Galaxies: kinematics and dynamics; Galaxies: star clusters; Methods: N body simulations

Indexed keywords

FRICTION; GALAXIES; STARS; TRIBOLOGY;

DWARF GALAXIES; DYNAMICAL FRICTIONS; GALAXIES: DWARF; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES: STAR CLUSTERS; LOCAL GROUPS; MASS LOSS; METHODS:N-BODY SIMULATIONS; STAR CLUSTERS; STELLAR SYSTEM;

ORBITS;

EID: 33846962850     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11308.x     Document Type: Article

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