Can bars be destroyed by a central mass concentration? - I. Simulations

Monthly Notices of the Royal Astronomical Society

Volumn 363, Issue 2, 2005, Pages 496-508

  Athanassoula, E ^a   Lambert, J C ^a   Dehnen, W ^b  

^a OBSERVATOIRE DE MARSEILLE   (France)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

Author keywords

Galaxies: bulges; Galaxies: evolution; Galaxies: kinematics and dynamics; Galaxies: structure; Methods: N body simulations

Indexed keywords

BLACK HOLES;

DENSITY PROFILE; DISK GALAXIES; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES:STRUCTURE; GALAXY EVOLUTION; GALAXY:BULGE; MASS CONCENTRATION; METHODS:N-BODY SIMULATIONS; SECULAR EVOLUTION; SURFACE DENSITY;

GALAXIES;

EID: 27144514968     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09445.x     Document Type: Article

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