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Orbital structure of triaxial galaxies

Published online by Cambridge University Press:  26 May 2016

Glenn van de Ven ,
Ellen Verolme ,
Michele Cappellari  and
Tim de Zeeuw
Glenn van de Ven
Affiliation:
Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, the Netherlands
Ellen Verolme
Affiliation:
Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, the Netherlands
Michele Cappellari
Affiliation:
Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, the Netherlands
Tim de Zeeuw
Affiliation:
Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, the Netherlands

Abstract

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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.

Type
Part 5: Clusters and Ellipticals
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 179 - 180
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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