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

dc.creatorBrunini, Adrian
dc.date.accessioned2019-03-26T21:32:04Z
dc.date.accessioned2022-10-15T07:13:09Z
dc.date.available2019-03-26T21:32:04Z
dc.date.available2022-10-15T07:13:09Z
dc.date.created2019-03-26T21:32:04Z
dc.date.issued2017-03
dc.identifierBrunini, 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; 3949-3955
dc.identifier0035-8711
dc.identifierhttp://hdl.handle.net/11336/72603
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4359203
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.
dc.languageeng
dc.publisherWiley Blackwell Publishing, Inc
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/465/4/3949/2568841?redirectedFrom=fulltext
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stw3043
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectASTEROIDS: GENERAL
dc.subjectMINOR PLANETS
dc.titleOrigin of slow-rotating minor bodies by tidal decoupling of binary pairs
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


Este ítem pertenece a la siguiente institución