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dc.contributor.authorCallegari, N.
dc.contributor.authorFerrazMello, S.
dc.contributor.authorMichtchenko, T. A.
dc.date.accessioned2014-02-26T17:25:20Z
dc.date.accessioned2014-05-20T14:16:07Z
dc.date.available2014-02-26T17:25:20Z
dc.date.available2014-05-20T14:16:07Z
dc.date.issued2006-04-01
dc.identifierhttp://dx.doi.org/10.1007/s10569-006-9002-4
dc.identifier.citationCelestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006.
dc.identifier.issn0923-2958
dc.identifier.urihttp://hdl.handle.net/11449/24846
dc.description.abstractThis paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar problem, is used and the solutions are analyzed through surfaces of section and Fourier techniques in the full phase space of the system.en
dc.format.extent381-397
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofCelestial Mechanics & Dynamical Astronomy
dc.sourceWeb of Science
dc.subjectchaospt
dc.subjectextra-solar planetspt
dc.subjectplanetary systemspt
dc.subjectpulsar planetspt
dc.subjectresonancept
dc.titleDynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12en
dc.typeArtigo
dcterms.licensehttp://www.springer.com/open+access/authors+rights?SGWID=0-176704-12-683201-0
dcterms.rightsHolderSpringer
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.description.affiliationUNESP, DEMAC, Rio Claro, Brazil
dc.description.affiliationUniv São Paulo, Inst Astron Geofis & Ciências Atmosfer, São Paulo, Brazil
dc.description.affiliationUnespUNESP, DEMAC, Rio Claro, Brazil
dc.identifier.doi10.1007/s10569-006-9002-4
dc.identifier.wosWOS:000238517200002
dc.rights.accessRightsAcesso restrito
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Geociências e Ciências Exatas, Rio Claropt
dc.relation.ispartofjcr2.121
dc.relation.ispartofsjr1,092
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