Abstract
This paper is devoted to radial orbit instability in the context of self-gravitating dynamical systems. We present this instability in the new frame of dissipation-induced instability theory. This allows us to obtain a rather simple proof based on energetics arguments and to clarify the associated physical mechanism.
| Original language | English |
|---|---|
| Pages (from-to) | 2785-2790 |
| Number of pages | 6 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 405 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 1 Jan 2010 |
Keywords
- Gravitation
- Instabilities
- Methods: analytical
- Stars: kinematics and dynamics
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