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Calculation of Perturbations in the Stellar Three-Body Problem
Published online by Cambridge University Press: 12 April 2016
Abstract
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The method of perturbations of Deprit has been applied to the stellar three-body problem. The calculation, developed previously by the authors in other articles, is here systematicized for easy use and applied to various triple systems.
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- Copyright © Astronomical Society of the Pacific 1992
References
Abad, A.J.
1984, Estudio de Sistemas Estelares Múltiples. Pub. Seminario Garcia Galdeano, Ser. II, Sec. 2, num. 2, Universidad de Zaragoza. Spain
Google Scholar
Deprit, A.
1969, Canonical Transformatione Depending on a Small Parameter, Celes. Mech.
1, 12
Google Scholar
Docobo, J.A.
1977, Aplicación de la teoría de Perturbaciones al estudio de sistemas estelares triples. Tesis Doctoral. Universidad de Zaragoza
Google Scholar
Docobo, J.A. & Prieto, C.
1988, The Stellar Three-body Problem. Explicit Formulation for Computing Perturbations. Pub. Obs. Ast. R.M. Aller
46
Google Scholar
Harrington, R.S.
1968b, Dynamics of the Triple System Zeta Aquarii, AJ, 73, 508
CrossRefGoogle Scholar
Heintz, W.D.
1967, Storungen und Bahnelemente im System Ursae Majoris, Astrom. Nach.
289-6, 269
CrossRefGoogle Scholar
Ling, J.F.
1989, Aplicación del método estroboscópico al problema estelar de tres cuerpos. Tesis Doctoral. Universidad de Santiago
Google Scholar
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