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.Comment: 2 pages (1 figure), to appear in the proceedings of the IAU Symposium
220 "Dark matter in galaxies", eds. S. Ryder, D.J. Pisano, M. Walker and K.
Freema