Motion Around A Monopole + Ring System - I. Stability Of Equatorial Circular Orbits Versus Regularity Of Three-dimensional Motion

dc.creatorRamos-Caro J.
dc.creatorPedraza J.F.
dc.creatorLetelier P.S.
dc.date2011
dc.date2015-06-30T20:30:59Z
dc.date2015-11-26T14:50:45Z
dc.date2015-06-30T20:30:59Z
dc.date2015-11-26T14:50:45Z
dc.date.accessioned2018-03-28T22:02:03Z
dc.date.available2018-03-28T22:02:03Z
dc.identifier
dc.identifierMonthly Notices Of The Royal Astronomical Society. , v. 414, n. 4, p. 3105 - 3116, 2011.
dc.identifier358711
dc.identifier10.1111/j.1365-2966.2011.18618.x
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-79959822297&partnerID=40&md5=4d6fae1f77d1610f15706b8ea39bd755
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/108187
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/108187
dc.identifier2-s2.0-79959822297
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1254253
dc.descriptionWe study the motion of test particles around a centre of attraction represented by a monopole (with and without spheroidal deformation) surrounded by a ring, given as a superposition of Morgan and Morgan discs. We deal with two kinds of bounded orbits: (i) equatorial circular orbits and (ii) general three-dimensional orbits. The first case provides a method to perform a linear stability analysis of these structures by studying the behaviour of vertical and epicyclic frequencies as functions of the mass ratio, the size of the ring and/or the quadrupolar deformation. In the second case, we study the influence of these parameters in the regularity or chaoticity of motion. We find that there is a close connection between linear stability (or instability) of equatorial circular orbits and regularity (or chaoticity) of the three-dimensional motion. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.
dc.description414
dc.description4
dc.description3105
dc.description3116
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dc.languageen
dc.publisher
dc.relationMonthly Notices of the Royal Astronomical Society
dc.rightsaberto
dc.sourceScopus
dc.titleMotion Around A Monopole + Ring System - I. Stability Of Equatorial Circular Orbits Versus Regularity Of Three-dimensional Motion
dc.typeArtículos de revistas


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