The high-eccentricity asymmetric expansion of the disturbing function for non-planar resonant problems

dc.contributorUniversidade de São Paulo (USP)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T15:25:12Z
dc.date.available2014-05-20T15:25:12Z
dc.date.created2014-05-20T15:25:12Z
dc.date.issued1998-01-01
dc.identifierAstronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 329, n. 1, p. 339-349, 1998.
dc.identifier0004-6361
dc.identifierhttp://hdl.handle.net/11449/35656
dc.identifierWOS:000071079700041
dc.identifierWOS000071079700041.pdf
dc.description.abstractIn this paper we present an extension to the nonplanar case of the asymmetric expansion of the averaged resonant disturbing function of Ferraz-Mello & Sato (1989, A&A 225, 541-547). Comparions with the exact averaged disturbing function are also presented. The expansion gives a good approximation of the exact function in a wide region around the center of expansion.
dc.languageeng
dc.publisherEdp Sciences S A
dc.relationAstronomy & Astrophysics
dc.relation2,265
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectcelestial mechanics
dc.subjectsolar system : general
dc.subjectmethods : analytical
dc.titleThe high-eccentricity asymmetric expansion of the disturbing function for non-planar resonant problems
dc.typeArtículos de revistas


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