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

dc.contributor.authorRoig, F.
dc.contributor.authorSimula, A.
dc.contributor.authorFerraz-Mello, S.
dc.contributor.authorTsuchida, M. [UNESP]
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-04-28T18:53:20Z
dc.date.available2022-04-28T18:53:20Z
dc.date.issued1998-01-01
dc.description.abstractIn this paper we present an extension to the non-planar 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.en
dc.description.affiliationInst. Astron. e Geofísico. Universidade de São Paulo, Av. Miguel Stéfano, 4200 São Paulo, SP
dc.description.affiliationInst. de Biociências Letras e Ciências Exatas Universidade Estadual Paulista, Sao Jose do Rio Preto, SP
dc.description.affiliationUnespInst. de Biociências Letras e Ciências Exatas Universidade Estadual Paulista, Sao Jose do Rio Preto, SP
dc.format.extent339-349
dc.identifier.citationAstronomy and Astrophysics, v. 329, n. 1, p. 339-349, 1998.
dc.identifier.issn0004-6361
dc.identifier.scopus2-s2.0-0006806172
dc.identifier.urihttp://hdl.handle.net/11449/219008
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.sourceScopus
dc.subjectCelestial mechanics solar system: general
dc.subjectMethods: analytical
dc.titleThe high-eccentricity asymmetric expansion of the disturbing function for non-planar resonant problemsen
dc.typeArtigo

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