Stable planetary orbits around one component in nearby binary stars-Reference-Cited by-同舟云学术

Stable planetary orbits around one component in nearby binary stars

Published:1987-03 Issue:1-4 Volume:43 Page:47-53
ISSN:0008-8714
Container-title:Celestial Mechanics
language:en
Short-container-title:Celestial Mechanics

Author:

Benest D.

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/BF01234553.pdf

Reference39 articles.

1. Aumann, H.H.: 1985, ?Protoplanetary material around nearby stars?, inThe search for extraterrestrial life: recent developments, ed. M.Papagiannis (Reidel), pp. 43?50.

2. Belyaev, N.A., Kresak, L., Pittich, E.M., Pushkarev, A.N.: 1986,Catalogue of short-period comets, Slovak Acad. Sci. Bratislava.

3. Benest, D.: 1971, ?Elliptic Restricted Problem for Sun-Jupiter: Existence of Stable Retrograde Satellites at Large Distance.?,Astron. Astrophys.,13,157?160.

4. Benest, D.: 1974/1975/1976, ?Effects of the Mass Ratio on the Existence of Retrograde Satellites in the Circular Plane Restricted Problem I/II/III?,Astron. Astrophys.,32,39?46/45,353?363/53,231?236.

5. Benest, D.: 1979, ?Derniers Résultats dans l'Etude du Problème Restreint.?, inMécanique Céleste, Astrométric et Géodésie, ed.GS5 (Obs.Bordeaux), p. 23.

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