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dc.contributor.authorCarruba, V.-
dc.contributor.authorHuaman, M. E.-
dc.contributor.authorDomingos, R. C.-
dc.contributor.authorDos Santos, C. R.-
dc.contributor.authorSouami, D.-
dc.date.accessioned2014-12-03T13:09:14Z-
dc.date.accessioned2016-10-25T20:10:27Z-
dc.date.available2014-12-03T13:09:14Z-
dc.date.available2016-10-25T20:10:27Z-
dc.date.issued2014-04-01-
dc.identifierhttp://dx.doi.org/10.1093/mnras/stu192-
dc.identifier.citationMonthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 439, n. 3, p. 3168-3179, 2014.-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/11449/112112-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/112112-
dc.description.abstractThe origin of this large population of V-type objects is not well understood. Since it seems unlikely that Vestoids crossing the 3J:-1A mean-motion resonance with Jupiter could account for the whole population of V-type asteroids in the central and outer main belt, origin from local sources, such as the parent bodies of the Eunomia, and of the Merxia and Agnia asteroid families, has been proposed as an alternative mechanism.In this work, we investigated the dynamical evolution of the V-type photometric candidates in the central main belt, under the effect of gravitational and non-gravitational forces. Our results show that dynamical evolution from the parent bodies of the Eunomia and Merxia/Agnia families on time-scales of 2 Byr or more could be responsible for the current orbital location of most of the low-inclined V-type asteroids.en
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.description.sponsorshipNational Aeronautics and Space Administration-
dc.description.sponsorshipPlanetary Science Division of the National Aeronautics and Space Administration-
dc.format.extent3168-3179-
dc.language.isoeng-
dc.publisherOxford University Press-
dc.sourceWeb of Science-
dc.subjectcelestial mechanicsen
dc.subjectminor planetsen
dc.subjectasteroids: generalen
dc.titleDynamical evolution of V-type asteroids in the central main belten
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionInstituto Nacional de Pesquisas Espaciais (INPE)-
dc.contributor.institutionUniv Namur-
dc.contributor.institutionUniv Paris 06-
dc.description.affiliationUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil-
dc.description.affiliationInst Nacl Pesquisas Espaciais, BR-12227010 So Jos Dos Campos, SP, Brazil-
dc.description.affiliationUniv Namur, Dept Math, Namur Ctr Complex Syst, NAXYS, B-5000 Namur, Belgium-
dc.description.affiliationUniv Paris 06, F-75005 Paris, France-
dc.description.affiliationUniv Paris 06, CNRS, UMR 8630, Observ Paris,SYRTE, F-75005 Paris, France-
dc.description.affiliationUnespUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil-
dc.description.sponsorshipIdFAPESP: 11/19863-3-
dc.description.sponsorshipIdCNPq: 305453/2011-4-
dc.identifier.doi10.1093/mnras/stu192-
dc.identifier.wosWOS:000334114900077-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
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