Simulations of the Eccentric Nuclear Disk in M31

Details Simulations of the Eccentric Nuclear Disk in M31 Simulations of the Eccentric Nuclear Disk in M31

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..275..277s&link_type=abstract

Disks of Galaxies: Kinematics, Dynamics and Peturbations, ASP Conference Proceedings, Vol. 275. Edited by E. Athanassoula, A. Bo

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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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