Abstract
The evolution of one-dimensional two-phase-space-density selfgravitating systems of stars is investigated by following the motion of the boundary curves of the systems in phase space. A qualitative agreement with Lynden-Bell's theory predicting, for the most probably state, velocity dispersions inversely proportional to the phase space density of the component at the star formation, is found.
| Original language | English |
|---|---|
| Pages (from-to) | 425-445 |
| Number of pages | 21 |
| Journal | Astrophysics and Space Science |
| Volume | 13 |
| Issue number | 2 |
| DOIs | |
| State | Published - Oct 1971 |