Dynamical evolution of V-type photometric candidates in the outer main belt

Registro completo de metadados
MetadadosDescriçãoIdioma
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.creatorHuaman, M. E.-
Autor(es): dc.creatorCarruba, V.-
Autor(es): dc.creatorDomingos, R. C.-
Data de aceite: dc.date.accessioned2021-03-10T21:31:57Z-
Data de disponibilização: dc.date.available2021-03-10T21:31:57Z-
Data de envio: dc.date.issued2015-03-18-
Data de envio: dc.date.issued2015-03-18-
Data de envio: dc.date.issued2014-11-01-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1093/mnras/stu1655-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/117003-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/117003-
Descrição: dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
Descrição: dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
Descrição: dc.descriptionNational Aeronautics and Space Administration-
Descrição: dc.descriptionPlanetary Science Division of the National Aeronautics and Space Administration-
Descrição: dc.descriptionProcesso FAPESP: 11/19863-3-
Descrição: dc.descriptionCNPq: 305453/2011-4-
Descrição: dc.descriptionV-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.-
Formato: dc.format2985-2992-
Idioma: dc.languageen-
Publicador: dc.publisherOxford Univ Press-
Relação: dc.relationMonthly Notices Of The Royal Astronomical Society-
Relação: dc.relation5.194-
Relação: dc.relation2,346-
Direitos: dc.rightsclosedAccess-
Palavras-chave: dc.subjectcelestial mechanics-
Palavras-chave: dc.subjectminor planets, asteroids: general-
Título: dc.titleDynamical evolution of V-type photometric candidates in the outer main belt-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

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