Please use this identifier to cite or link to this item: https://hdl.handle.net/10953/1584
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dc.contributor.authorGarrido, J.L.-
dc.contributor.authorBattaner, E.-
dc.contributor.authorSánchez-Saavedra, M.L.-
dc.contributor.authorFlorido, E.-
dc.date.accessioned2024-01-22T22:55:02Z-
dc.date.available2024-01-22T22:55:02Z-
dc.date.issued1993-04-
dc.identifier.issn0004-6361es_ES
dc.identifier.urihttps://ui.adsabs.harvard.edu/abs/1993A&A...271...84Ges_ES
dc.identifier.urihttps://hdl.handle.net/10953/1584-
dc.description.abstractThe method of convergence of planes developed by Battaner et al. (1991, hereafter BGSF) has been used for investigating coherent alignments of rotation axes of spiral galaxies in the Milky Way neighbourhood. Results are contrasted with previous analyses carried out by other means, taking into account that they were not conclusive either to confirm or to reject coherent alignments. Some improvements of the method are described. No evidence for coherent alignments has been found here, with the exception of some zones, in particular that around the Coma supercluster in which the angular momentum vectors tend to be perpendicular to the axis of the Coma supercluster.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.relation.ispartofAstronomy and Astrophysics, Vol. 271, p. 84-88 (1993)es_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.subjectgalaxies: spirales_ES
dc.subjectgalaxies: clusteringes_ES
dc.subjectgalaxies: formationes_ES
dc.subjectmethods: statisticales_ES
dc.titleOn the coherent orientation of spins of spiral galaxieses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.subject.udc5es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.type.versioninfo:eu-repo/semantics/acceptedVersiones_ES
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