Fractal analysis of galaxy surveys

dc.contributor.author	Seshadri, T. R
dc.date.accessioned	2006-03-14T04:30:54Z
dc.date.available	2006-03-14T04:30:54Z
dc.date.issued	2005-03
dc.identifier.citation	BASI, Vol. 33, No. 1, pp. 1-9	en
dc.identifier.uri	http://hdl.handle.net/2248 /747
dc.description.abstract	Fractal 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 Mpc	en
dc.format.extent	80279 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	cosmology	en
dc.subject	miscellaneous - cosmology	en
dc.subject	theory - methods	en
dc.subject	statistical - large-scale structure of the Universe	en
dc.title	Fractal analysis of galaxy surveys	en
dc.type	Article	en