The Stability of Perfect Elliptic Disks. I. The Maximum Streaming Case
Abstract
Self-consistent distribution functions are constructed for two- dimensional perfect elliptic disks (for which the potential is exactly integrable) in the limit of maximum streaming; these are tested for stability by N-body integration. To obtain a discrete representation for each model, simulated annealing is used to choose a set of orbits which sample the distribution function and reproduce the required density profile while carrying the greatest possible amount of angular momentum. A quiet start technique is developed to place particles on these orbits uniformly in action-angle space, making the initial conditions as smooth as possible. The roundest models exhibit spiral instabilities similar to those of cold axisymmetric disks; the most elongated models show bending instabilities like those seen in prolate systems. Between these extremes, there is a range of axial ratios 0.25 <~ b/a <~ 0.6 within which these models appear to be stable. All the methods developed in this investigation can easily be extended to integrable potentials in three dimensions.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- June 1994
- DOI:
- 10.1086/174262
- Bibcode:
- 1994ApJ...428..493L
- Keywords:
-
- Distribution Functions;
- Elliptic Functions;
- Elliptical Orbits;
- Galactic Structure;
- Lenticular Bodies;
- Many Body Problem;
- Stability;
- Two Dimensional Bodies;
- Annealing;
- Computerized Simulation;
- Elongation;
- Numerical Analysis;
- Prolateness;
- Astronomy;
- GALAXIES: ELLIPTICAL AND LENTICULAR;
- CD;
- GALAXIES: KINEMATICS AND DYNAMICS;
- GALAXIES: STRUCTURE;
- METHODS: ANALYTICAL;
- METHODS: NUMERICAL