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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2662
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dc.contributor.authorKrishan, V-
dc.contributor.authorSivaram, C-
dc.date.accessioned2008-07-14T06:16:14Z-
dc.date.available2008-07-14T06:16:14Z-
dc.date.issued1991-05-
dc.identifier.citationMonthly Notices of Royal Astronomical Society, Vol. 250, No.1, pp. 157 - 160en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2662-
dc.description.abstractA definite physical mechanism based in inverse cascading is suggested which quite naturally yields a bottom-up hierarchical structure for galactic clustering. In this mechanism, nonlinear interactions between small fluid elements in an energetically open nonlinear system facilitate the formation of large coherent stable structures. The clustering of galaxies on all scales is interpreted as the result of this self-organization processes occurring in a turbulent medium.en
dc.format.extent820689 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1991MNRAS.250..157Ken
dc.subjectAstronomical modelsen
dc.subjectCosmologyen
dc.subjectGalactic clustersen
dc.subjectNonlinear systemsen
dc.subjectTurbulent flowen
dc.subjectGravitational effectsen
dc.subjectKolmogoroff theoryen
dc.subjectRed shifen
dc.subjectSpatial distributionen
dc.subjectUniverseen
dc.titleClustering of galaxies by inverse cascade in a turbulent mediumen
dc.typeArticleen
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