Show simple item record

dc.contributor.authorHuaman, M. E. [UNESP]
dc.contributor.authorCarruba, V. [UNESP]
dc.contributor.authorDomingos, R. C. [UNESP]
dc.date.accessioned2015-03-18T15:54:43Z
dc.date.available2015-03-18T15:54:43Z
dc.date.issued2014-11-01
dc.identifierhttp://dx.doi.org/10.1093/mnras/stu1655
dc.identifier.citationMonthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 444, n. 3, p. 2985-2992, 2014.
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/11449/117003
dc.description.abstractV-type asteroids, characterized by two absorption bands at 1.0 and 2.0 mu m, are usually thought to be portions of the crust of differentiated or partially differentiated bodies. Most V-type asteroids are found in the inner main belt and are thought to be current or past members of the Vesta dynamical family. Recently, several V-type photometric candidates have been identified in the central and outer main belt. While the dynamical evolution of V-type photometric candidates in the central main belt has been recently investigated, less attention has been given to the orbital evolution of basaltic material in the outer main belt as a whole. Here, we identify known and new V-type photometric candidates in this region, and study their orbital evolution under the effect of gravitational and non-gravitational forces. A scenario in which a minimum of three local sources, possibly associated with the parent bodies of (349) Dembowska, (221) Eos, and (1459) Magnya, could in principle explain the current orbital distribution of V-type photometric candidates in the region.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.extent2985-2992
dc.language.isoeng
dc.publisherOxford Univ Press
dc.relation.ispartofMonthly Notices Of The Royal Astronomical Society
dc.sourceWeb of Science
dc.subjectcelestial mechanicsen
dc.subjectminor planets, asteroids: generalen
dc.titleDynamical evolution of V-type photometric candidates in the outer main belten
dc.typeArtigo
dcterms.licensehttp://www.oxfordjournals.org/access_purchase/self-archiving_policyb.html
dcterms.rightsHolderOxford Univ Press
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.description.affiliationUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.description.affiliationUniv Estadual Paulista, UNESP, BR-13874149 Sao Joao Da Boa Vista, SP, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, UNESP, BR-13874149 Sao Joao Da Boa Vista, SP, Brazil
dc.identifier.doi10.1093/mnras/stu1655
dc.identifier.wosWOS:000343399600073
dc.rights.accessRightsAcesso restrito
dc.description.sponsorshipIdFAPESP: 11/19863-3
dc.description.sponsorshipIdCNPq: 305453/2011-4
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
dc.identifier.lattes4750709016042276
unesp.author.lattes4750709016042276
dc.relation.ispartofjcr5.194
dc.relation.ispartofsjr2,346
Localize o texto completo

Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record