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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