Phase-space transport in cuspy triaxial potentials: Can they be used to construct self-consistent equilibria?

Monthly Notices of the Royal Astronomical Society

Volumn 319, Issue 1, 2000, Pages 43-62

  Siopis, Christos ^a,b   Kandrup, Henry E ^a,b,c  

^a University of Florida ^*  (United States)

^b OBSERVATOIRE DE MARSEILLE   (France)

^c UNIVERSITY OF FLORIDA   (United States)

Author keywords

Chaos; Galaxies: formation; Galaxies: kinematics and dynamics

Indexed keywords

BLACK HOLES; FRICTION; GALAXIES; LYAPUNOV METHODS; PHASE SPACE METHODS; STARS; TOYS;

AXISYMMETRY; CHAOTIC ORBITS; ELLIPTICALS; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY FORMATIONS; GENERALISATION; LOW-AMPLITUDE; PHASE SPACE TRANSPORT; SCHWARZSCHILD; STATISTICAL PROPERTIES;

GRAVITATION;

EID: 0002445944     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03740.x     Document Type: Article

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