Galaxy formation

dc.contributor.author	Padmanabhan, T
dc.contributor.author	Subramanian, K
dc.date.accessioned	2007-03-15T09:13:15Z
dc.date.available	2007-03-15T09:13:15Z
dc.date.issued	1992
dc.identifier.citation	BASI, Vol. 20, pp. 1-155	en
dc.identifier.uri	http://hdl.handle.net/2248/1453
dc.description.abstract	An attempt is made to develop a consistent theory describing galaxy formation. First, a discussion of the smooth universe is presented. The linear theory of perturbations is introduced, and its applications are described. Nonlinear evolution is then examined. The relevance of the high redshift universe to galaxy formation is discussed. Finally, consideration is given to the origin of density perturbations. The discussion emphasizes the theoretical aspects and physical basis for the models rather than detailed observational features or detailed examination of particular models	en
dc.format.extent	13236893 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Dark matter	en
dc.subject	Galatic evolution	en
dc.title	Galaxy formation	en
dc.type	Article	en