From rotations and inclinations to zero configurational velocity surfaces, II. The best possible configurational velocity surfaces-Reference-Cited by-同舟云学术

From rotations and inclinations to zero configurational velocity surfaces, II. The best possible configurational velocity surfaces

Published:1987-09 Issue:3-4 Volume:40 Page:197-223
ISSN:0008-8714
Container-title:Celestial Mechanics
language:en
Short-container-title:Celestial Mechanics

Author:

Saari Donald G.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine,Space and Planetary Science,Astronomy and Astrophysics,Applied Mathematics,Computational Mathematics,Mathematical Physics,Modeling and Simulation

Link

http://link.springer.com/content/pdf/10.1007/BF01235841.pdf

Reference18 articles.

1. Bozis, G.: 1976, ?Zero velocity surfaces for the general planar three body problem,?Astrophys. Space Sci. 43, 355?86.

2. Easton, R.: 1971, ?Some topology of the three body problem?.Jour. Diff. Eqs,10, 371?377.

3. Golubev, V.: 1967, ?Regions where motion is impossible in the three body problem,?Soviet Physics Doklady, 527?531.

4. Golubev, V.: 1968, ?Hill stability in the untrestricted three-body problem?,Soviet Physics-Doklady, 373?375.

5. Laskar, J. and Marchal, C.: 1984, ?Triple close approach in the three body problem: A limit for the bounded orbits,?Celest. Mech.,32, 15?28.

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