The Collective Relaxation of Two-Phase-Space-Density Collisions One-Dimensional Selfgravitating Systems (Part of the Proceedings of the IAU Colloquium No. 10, held in Cambridge, England, August 12-15, 1970.)

Details The Collective Relaxation of Two-Phase-Space-Density Collisions One-Dimensional Selfgravitating Systems (Part of the Proceedings of the IAU Colloquium No. 10, held in Cambridge, England, August 12-15, 1970.) The Collective Relaxation of Two-Phase-Space-Density Collisions One-Dimensional Selfgravitating Systems (Part of the Proceedings of the IAU Colloquium No. 10, held in Cambridge, England, August 12-15, 1970.)

Oct 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..13..425c&link_type=abstract

Astrophysics and Space Science, Volume 13, Issue 2, pp.425-445

Astronomy and Astrophysics

Astrophysics

9

Scientific paper

The evolution of one-dimensionaltwo-phase-space-density selfgravitating systems of stars is investigated by following the motion of the boundary curves of the systems in phase space. Aqualitative 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.

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