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| Paper: |
Eccentric Ring Dynamics: The M 31 Double Nucleus |
| Volume: |
197, XVth IAP Meeting Dynamics of Galaxies: From the Early Universe to the Present |
| Page: |
31 |
| Authors: |
Statler, T. S.; Salow, R.; Vine, S. |
| Abstract: |
The favored model for the nucleus of M31 consists of an eccentric disk with an off-center density concentration. If the disk is in equilibrium, the requirement that it precess uniformly under self-gravity creates an observable feature in the rotation curve, which may be visible in current HST data. |
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