Caustics of the restricted three-body problem

dc.contributorObserv Nacl
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade Federal de Viçosa (UFV)
dc.date.accessioned2014-05-20T15:25:09Z
dc.date.accessioned2022-10-05T16:31:56Z
dc.date.available2014-05-20T15:25:09Z
dc.date.available2022-10-05T16:31:56Z
dc.date.created2014-05-20T15:25:09Z
dc.date.issued1998-03-01
dc.identifierAstronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 331, n. 3, p. 1108-1112, 1998.
dc.identifier0004-6361
dc.identifierhttp://hdl.handle.net/11449/35621
dc.identifierWOS:000072713100046
dc.identifier0960024575647258
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3907521
dc.description.abstractTrajectories of the planar, circular, restricted three-body problem are given in the configuration space through the caustics associated to the invariant tori of quasi-periodic orbits. It is shown that the caustics of trajectories librating in any particular resonance display some features associated to that resonance. This method can be considered complementary to the Poincare surface of section method, because it provides information not accessible by the other method.
dc.languageeng
dc.publisherEdp Sciences S A
dc.relationAstronomy & Astrophysics
dc.relation2,265
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectcelestial mechanics, stellar dynamics
dc.subjectchaos
dc.titleCaustics of the restricted three-body problem
dc.typeArtigo


Este ítem pertenece a la siguiente institución