Abstract The dynamical evolution of a keplerian disk of matter around a star or around a planet is a crucial point for the understanding of the formation of solar systems or for the formation of planetary rings. In this paper we will adopt a general point of view : we describe the disk by a distribution function in phase space and follow its evolution in presence of a stochastic force or binary collisions.
Orbit perturbation: Evolution of a keplerian disk
Advances in Space Research ; 4 , 9 ; 95-105
1984-01-01
11 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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