Abstract
If a cosmological constant is accepted, at great distances, newtonian is modified in a Yukawa potential. There will then be a limit for stable circular orbits and then orbits of elliptic types. Moreover, the integrals to evoluate global effects of stellar encounters converge.
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References
Henon, H.: 1958, Ann. Astrophys. 21, 186–216.
Saslaw, W.C.: 1968, Monthly Notices Roy. Astron. Soc. 141, 71–108.
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© 1973 D. Reidel Publishing Company, Dordrecht-Holland
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Godart, O. (1973). Yukawa Potential and Stellar Encounter. In: Tapley, B.D., Szebehely, V. (eds) Recent Advances in Dynamical Astronomy. Astrophysics and Space Science Library, vol 39. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2611-6_23
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DOI: https://doi.org/10.1007/978-94-010-2611-6_23
Publisher Name: Springer, Dordrecht
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