Testing fundamental physics with distant star clusters: Theoretical models for pressure-supported stellar systems

Monthly Notices of the Royal Astronomical Society

Volumn 395, Issue 3, 2009, Pages 1549-1557

  Haghi, Hosein ^a,b   Baumgardt, Holger ^b   Kroupa, Pavel ^b   Grebel, Eva K ^c   Hilker, Michael ^d   Jordi, Katrin ^c  

^a INSTITUTE FOR ADVANCED STUDIES IN BASIC SCIENCES IASBS   (Iran)

^b UNIVERSITY OF BONN   (Germany)

^c ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxies: clusters: general; Galaxies: dwarf; Gravitation; Methods: analytical; Methods: N body simulations

Indexed keywords

DISPERSIONS; GALAXIES; STARS; VELOCITY;

FUNDAMENTAL PHYSICS; GALAXIES: CLUSTERS: GENERAL; GALAXIES: DWARF; GLOBULAR CLUSTERS; MEAN VELOCITIES; METHODS:ANALYTICAL; METHODS:N-BODY SIMULATIONS; NEWTONIAN DYNAMICS; STELLAR SYSTEM; VELOCITY DISPERSION;

GRAVITATION;

EID: 65649083729     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14656.x     Document Type: Article

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