A counterpart to the radial-orbit instability in triaxial stellar systems

Monthly Notices of the Royal Astronomical Society

Volumn 399, Issue 2, 2009, Pages 671-682

  Antonini, F ^a,b   Capuzzo Dolcetta, R ^b   Merritt, D ^a  

^a ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

Author keywords

Dark matter; Galaxies: elliptical and lenticular, cD; Methods: numerical; Stellar dynamics

Indexed keywords

GALAXIES; NUMERICAL METHODS; STARS;

DARK MATTER; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXY MODELS; MASS MODELS; METHOD: NUMERICAL; SELF-CONSISTENT SOLUTION; STEADY STATE; STELLAR DYNAMICS; STELLAR SYSTEM; TRIAXIAL MODELING;

STABILITY;

EID: 70349866530     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15342.x     Document Type: Article

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