A Dynamical N-body model for the central region of ω Centauri

Astronomy and Astrophysics

Volumn 538, Issue , 2012, Pages

  Jalali, B ^a   Baumgardt, H ^b,c   Kissler Patig, M ^a   Gebhardt, K ^d   Noyola, E ^e,f   Lutzgendorf N ^a   De Zeeuw, P T ^a,g  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b UNIVERSITY OF BONN   (Germany)

^c UNIVERSITY OF QUEENSLAND   (Australia)

^d The University of Texas at Austin   (United States)

^e UNIVERSITY OF MUNICH   (Germany)

^f UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^g LEIDEN UNIVERSITY   (Netherlands)

Author keywords

black hole physics; Galaxy: kinematics and dynamics; globular clusters: individual: Centauri; methods: numerical

Indexed keywords

BEST-FIT MODELS; BLACK HOLE PHYSICS; BLACK HOLES; CORE RADIUS; DATA SETS; DYNAMICAL EVOLUTION; GALACTIC STARS; GALAXY: KINEMATICS AND DYNAMICS; GLOBULAR CLUSTERS; HIGH VELOCITY; HOST GALAXIES; IDEAL SYSTEMS; INITIAL CONDITIONS; INITIAL PARAMETER; LOW MASS; METHODS: NUMERICALS; N-BODY SIMULATION; PROPER MOTION; RADIAL VELOCITY; SPECIAL-PURPOSE COMPUTER; SPHERICAL MODELS; STAR CLUSTERS; STELLAR MASS; STELLAR POPULATIONS; STRUCTURE AND DYNAMICS; SUPERMASSIVE BLACK HOLES; SURFACE BRIGHTNESS; VELOCITY DISPERSION;

COMPUTER SIMULATION; DYNAMICS; GALAXIES; GRAVITATION; KINEMATICS; LUMINANCE; STARS; VELOCITY;

DISPERSIONS;

EID: 84856405497     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116923     Document Type: Article

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