Triaxial orbit based galaxy models with an application to the (apparent) decoupled core galaxy NGC 4365

Monthly Notices of the Royal Astronomical Society

Volumn 385, Issue 2, 2008, Pages 647-666

  Van Den Bosch, R C E ^a   Van De Ven, G ^a,b,c   Verolme, E K ^a,d   Cappellari, M ^a,e   De Zeeuw, P T ^a,f  

^a LEIDEN UNIVERSITY   (Netherlands)

^b PRINCETON UNIVERSITY   (United States)

^c INSTITUTE FOR ADVANCED STUDY   (United States)

^d TNO   (Netherlands)

^e UNIVERSITY OF OXFORD   (United Kingdom)

^f EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxies: elliptical and lenticular, cD; Galaxies: kinematics and dynamics; Galaxies: structure

Indexed keywords

DISTRIBUTION FUNCTIONS; LUMINANCE; PHASE SPACE METHODS;

AM GENERALS; BLACK HOLES; DYNAMICAL MODELING; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES:STRUCTURE; GALAXY MODELS; LUMINOSITY DISTRIBUTIONS; ORBITALS; SCHWARZSCHILD;

GALAXIES;

EID: 40549108966     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.12874.x     Document Type: Article

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