What determines the strength and the slowdown rate of bars?

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 4, 2003, Pages 1179-1198

  Athanassoula, E ^a  

^a OBSERVATOIRE DE MARSEILLE   (France)

Author keywords

Galaxies: evolution galaxies: structure; Galaxies: kinematics and dynamics; Methods: numerical

Indexed keywords

ANGULAR DISTRIBUTION; ANGULAR MOMENTUM; DISPERSIONS; NUMERICAL METHODS;

AT RESONANCE; DISTRIBUTION-FUNCTIONS; EVOLUTION - GALAXY; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES:STRUCTURE; GALAXY EVOLUTION; GALAXY: EVOLUTION GALAXY: STRUCTURE; METHOD: NUMERICAL; RESONANT MATERIALS; VELOCITY DISPERSION;

GALAXIES;

EID: 0141430424     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06473.x     Document Type: Article

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