English

Building Self-Consistent Triaxial Galaxy Models Using Schwarzschild's Method

Astrophysics 2007-05-23 v1

Abstract

We use Schwarzschild's orbit superposition method to build self-consistent models of elliptical galaxies with scale-free potentials. Our exhaustive study of all physical shapes and central densities for galaxies with scale-free potentials establishes a relationship between the presence of chaos and self-consistency. The extent and the onset of chaos is studied by varying parameters of the model which are believed to be its inducers, such as the steepness of the central density cusp, flatness and triaxiality. We show that gravitational scattering of the central density cusp plays a dominant role in restricting the shapes of elliptical galaxies.

Keywords

Cite

@article{arxiv.astro-ph/0305005,
  title  = {Building Self-Consistent Triaxial Galaxy Models Using Schwarzschild's Method},
  author = {Balsa Terzic},
  journal= {arXiv preprint arXiv:astro-ph/0305005},
  year   = {2007}
}

Comments

19 pages, 12 figures; submitted to ApJ