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dc.date.accessioned 2020-04-17T12:48:49Z
dc.date.available 2020-04-17T12:48:49Z
dc.date.issued 2012-01
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/93622
dc.description.abstract Orbits in the principal planes of triaxial potentials are known to be prone to unstable motion normal to those planes, so that three dimensional investigations of those orbits are needed even though they are two dimensional. We present here an investigation of such orbits in the well known logarithmic potential which shows that the third dimension must be taken into account when studying them and that the instability worsens for lower values of the forces normal to the plane. Partially chaotic orbits are present around resonances, but also in other regions. The action normal to the plane seems to be related to the isolating integral that distinguishes regular from partially chaotic orbits, but not to the integral that distinguishes partially from fully chaotic orbits. en
dc.format.extent 107-115 es
dc.language en es
dc.subject Chaotic motions es
dc.subject Stellar systems es
dc.subject Stability es
dc.subject Partially chaotic orbits es
dc.subject Logarithmic potential es
dc.title A three dimensional investigation of two dimensional orbits en
dc.type Articulo es
sedici.identifier.other http://dx.doi.org/10.1007/s10569-011-9388-5 es
sedici.identifier.other hdl:11336/42793 es
sedici.identifier.issn 0923-2958 es
sedici.creator.person Carpintero, Daniel Diego es
sedici.creator.person Muzzio, Juan Carlos es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Celestial Mechanics and Dynamical Astronomy es
sedici.relation.journalVolumeAndIssue vol. 112, no. 1 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)