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.


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    Title :

    Orbit perturbation: Evolution of a keplerian disk


    Contributors:
    Pellat, R. (author) / Barge, P. (author) / Hornung, P. (author) / Millet, J.M. (author)

    Published in:

    Publication date :

    1984-01-01


    Size :

    11 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English




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