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The Effect of Non-Stationary Action on the Motion of Particles in Protoplanetary Nebulae

Published online by Cambridge University Press:  07 August 2017

A.S. Baranov
A.S. Baranov*
Affiliation:
Institute of Theoretical Astronomy, USSR Academy of Sciences, 10 Kutuzov Quay, St. Petersburg, 191187, USSR

Extract

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Dynamical evolution of a plane system of non-interacting particles, which are in a certain smoothed-out regular field, is of a certain interest in a number astronomical applications. Among them are the plane subsystems of the spiral galaxies, the rings of the giant planets and protoplanetary nebulae. The problem of determining the stationary state of these systems has been studied enough [1]. But one seldom comes across studies concerning with the reaction of the non-stationary field.

Type
Part VI - Meteors. Zodiacal Cloud. Nebulae
Information
Symposium - International Astronomical Union , Volume 152: Chaos, Resonance and Collective Dynamical Phenomena in the Solar System , 1992 , pp. 359 - 362
Copyright
Copyright © Kluwer 1992 

References

1. Polyachenko, V.L. and Fridman, A.M.: 1976, Equilibrium and Stability of Gravitating Systems , Nauka, Moscow (in Russian).Google Scholar
2. Lichtenberg, A.J. and Lieberman, M.A.: 1983, Regular and Stochastic Motion , Springer-Verlag, Berlin-Heidelberg-New-York.CrossRefGoogle Scholar
3. Zaslavsky, G.M., Sagdeev, R.Z., Usikov, D.A., Chernikov, A.A.: 1991, Weak Chaos and Quasi-Regular Patterns , Nauka, Moscow (in Russian).CrossRefGoogle Scholar