Orbital structure of triaxial galaxies
Glenn van de Ven, Ellen Verolme, Michele Cappellari, Tim de Zeeuw
Abstract
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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