Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade de São Paulo (USP)
dc.date.accessioned2014-02-26T17:25:20Z
dc.date.accessioned2014-05-20T14:16:07Z
dc.date.accessioned2022-10-05T15:10:59Z
dc.date.available2014-02-26T17:25:20Z
dc.date.available2014-05-20T14:16:07Z
dc.date.available2022-10-05T15:10:59Z
dc.date.created2014-02-26T17:25:20Z
dc.date.created2014-05-20T14:16:07Z
dc.date.issued2006-04-01
dc.identifierCelestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006.
dc.identifier0923-2958
dc.identifierhttp://hdl.handle.net/11449/24846
dc.identifier10.1007/s10569-006-9002-4
dc.identifierWOS:000238517200002
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3898023
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.
dc.languageeng
dc.publisherSpringer
dc.relationCelestial Mechanics & Dynamical Astronomy
dc.relation2.121
dc.relation1,092
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectchaos
dc.subjectextra-solar planets
dc.subjectplanetary systems
dc.subjectpulsar planets
dc.subjectresonance
dc.titleDynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12
dc.typeArtigo


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