Orbital structure of triaxial galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages (1 figure), to appear in the proceedings of the IAU Symposium 220 "Dark matter in galaxies", eds. S. Ryder, D.J. Pisan

Scientific paper

We have developed a method to construct realistic triaxial dynamical models
for elliptical galaxies, allowing us to derive best-fitting parameters, such as
the mass-to-light ratio and the black hole mass, and to study the orbital
structure. We use triaxial theoretical Abel models to investigate the
robustness of the method.

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