Origin of slow-rotating minor bodies by tidal decoupling of binary pairs

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dc.conicet.comentariosArtículo incompletoes
dc.conicet.fuenteindividual
dc.conicet.organizacionConsejo Nacional de Investigaciones Científicas y Técnicas
dc.conicet.organizacionUniversidad Nacional de la Patagonia Austral. Unidad Académica Caleta Olivia. Departamento de Ciencias Exactas y Naturales
dc.conicet.paisOrganizacionArgentina
dc.conicet.paisOrganizacionArgentina
dc.conicet.produccionid7385730
dc.contributor.authorBrunini, Adrian
dc.date.accessioned2019-03-26T21:32:04Z
dc.date.available2019-03-26T21:32:04Z
dc.date.issued2017-03
dc.date.updated2019-03-26T14:08:36Z
dc.description.abstractIn this paper, we show that the decoupling of binary pairs by tidal interaction and Kozai oscillations acting together can generate single objects in a slow-rotation-rate state. This mechanism has the merit of not being strongly dependent on the size or shape of the objects. The key parameter leading the process is ω/n, the ratio between the rotation rate and the orbital mean motion of the binary, which must be > 1. The proposed mechanism could also operate in other populations of minor bodies.es
dc.description.filFil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Patagonia Austral. Unidad Académica Caleta Olivia. Departamento de Ciencias Exactas y Naturales; Argentina
dc.formatapplication/pdfes
dc.identifier.citationBrunini, Adrian; Origin of slow-rotating minor bodies by tidal decoupling of binary pairs; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 465; 4; 3-2017; 3949-3955es
dc.identifier.institucionalCONICET
dc.identifier.issn0035-8711es
dc.identifier.repoCONICET Digital
dc.identifier.urihttp://hdl.handle.net/11336/72603
dc.journal.ciudadLondreses
dc.journal.number4es
dc.journal.pagination3949-3955es
dc.journal.paisReino Unidoes
dc.journal.titleMonthly Notices of the Royal Astronomical Societyes
dc.journal.volume465es
dc.language.isoenges
dc.publisherWiley Blackwell Publishing, Inces
dc.relation.alternativeidinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/465/4/3949/2568841?redirectedFrom=fulltext
dc.relation.alternativeidinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stw3043
dc.rightsinfo:eu-repo/semantics/openAccess*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/*
dc.subjectAsteroids: Generales
dc.subjectMinor Planetses
dc.subject.classificationAstronomíaes
dc.subject.classificationCiencias Físicases
dc.subject.classificationCIENCIAS NATURALES Y EXACTASes
dc.titleOrigin of slow-rotating minor bodies by tidal decoupling of binary pairses
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion

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