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| Paper: |
Simulations of the Eccentric Nuclear Disk in M31 |
| Volume: |
275, Disks of Galaxies: Kinematics, Dynamics and Perturbations |
| Page: |
277 |
| Authors: |
Salow, R. M. |
| Abstract: |
We have constructed approximate self-consistent models of eccentric stellar disks around central black holes. (Salow & Statler 2001). Disks are built using a distribution function (DF) which approximates quasiperiodic orbits as dispersed Kepler ellipses. The models have properties which produce observables strikingly similar to those seen in the double nucleus of M31. |
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