Mathematics
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...279..610r&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 279, April 15, 1984, p. 610-620.
Mathematics
17
Celestial Mechanics, Equations Of Motion, Orbit Calculation, Stellar Motions, Stellar Orbits, Algorithms, Iteration, Partial Differential Equations, Transformations (Mathematics)
Scientific paper
Following recent basic developments by Binney and Spergel, the equations of motion for a star in a galactic potential have been transformed from time to angle variables. A numerical procedure has been devised to solve the transformed equations for two-dimensional box and loop orbits in the equatorial plane of a triaxial potential. In this procedure an orbit is specified not by its starting values in phase space, but either by its frequencies or by its action values. A substantial set of orbits has been derived by this procedure for one potential. The results for their physical and geometrical characteristics are displayed in action diagrams.
Chang K. M.
Ratcliff Stephen J.
Schwarzschild Martin
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