1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2678
Full metadata record
DC FieldValueLanguage
dc.contributor.authorKrishan, V-
dc.date.accessioned2008-07-14T09:12:59Z-
dc.date.available2008-07-14T09:12:59Z-
dc.date.issued1993-09-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 264, No. 1, pp. 257 - 260en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2678-
dc.description.abstractThe development of large-scale flows from the stresses generated by small-scale flows in a Navier-Stokes system is studied in order to model the large-scale structure of the Universe. This process is an analogue of the α-effect, by which a large-scale magnetic field can be generated beginning with small-scale fields. It is shown that, under similar conditions of anisotropy and non-zero mean helicity, large-scale flows can be generated. The clustering of galaxies on all possible scales is then suggested to be a result of the hydrodynamic hierarchy.en
dc.format.extent537191 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993MNRAS.264..257Ken
dc.subjectGalaxiesen
dc.subjectClustersen
dc.subjectMagnetic fielden
dc.titleClustering of Galaxies by the Alpha-Effecten
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
krish.pdf524.6 kBAdobe PDFView/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.