Conference item icon

Conference item

Orbital structure of triaxial galaxies

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.
Publication status:
Published

Actions


Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
DARK MATTER IN GALAXIES More from this journal
Issue:
220
Pages:
179-180
Publication date:
2004-01-01
Event title:
220th Symposium of the International-Astronomical-Union on Dark Matter in Galaxies held at the 25th IAU General Assembly
ISSN:
0074-1809
ISBN:
1583811672


Keywords:
Pubs id:
pubs:29600
UUID:
uuid:028cc564-21a4-4ab9-8cca-5acff7c521b8
Local pid:
pubs:29600
Source identifiers:
29600
Deposit date:
2012-12-19

Terms of use



Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP