Clustering of galaxies by inverse cascade in a turbulent medium

dc.contributor.author	Krishan, V
dc.contributor.author	Sivaram, C
dc.date.accessioned	2008-07-14T06:16:14Z
dc.date.available	2008-07-14T06:16:14Z
dc.date.issued	1991-05
dc.identifier.citation	Monthly Notices of Royal Astronomical Society, Vol. 250, No.1, pp. 157 - 160	en
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/2248/2662
dc.description.abstract	A 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.extent	820689 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1991MNRAS.250..157K	en
dc.subject	Astronomical models	en
dc.subject	Cosmology	en
dc.subject	Galactic clusters	en
dc.subject	Nonlinear systems	en
dc.subject	Turbulent flow	en
dc.subject	Gravitational effects	en
dc.subject	Kolmogoroff theory	en
dc.subject	Red shif	en
dc.subject	Spatial distribution	en
dc.subject	Universe	en
dc.title	Clustering of galaxies by inverse cascade in a turbulent medium	en
dc.type	Article	en