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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/747
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dc.contributor.authorSeshadri, T. R-
dc.date.accessioned2006-03-14T04:30:54Z-
dc.date.available2006-03-14T04:30:54Z-
dc.date.issued2005-03-
dc.identifier.citationBASI, Vol. 33, No. 1, pp. 1-9en
dc.identifier.urihttp://hdl.handle.net/2248 /747-
dc.description.abstractFractal analysis is a powerful tool to study the nature of galaxy distribution. The use of multifractal analysis of the galaxy distribution for the investigation of the transition to homogeneity in the Universe is reviewed. This analysis shows that the Universe is homogeneous over scales larger than about 80h-1 to 100h-1 Mpcen
dc.format.extent80279 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectcosmologyen
dc.subjectmiscellaneous - cosmologyen
dc.subjecttheory - methodsen
dc.subjectstatistical - large-scale structure of the Universeen
dc.titleFractal analysis of galaxy surveysen
dc.typeArticleen
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