Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1458
Full metadata record
DC FieldValueLanguage
dc.contributor.authorKapahi, V. K-
dc.date.accessioned2007-03-21T06:45:58Z-
dc.date.available2007-03-21T06:45:58Z-
dc.date.issued1992-
dc.identifier.citationBASI, Vol. 20, pp 49-60en
dc.identifier.urihttp://hdl.handle.net/2248/1458-
dc.description.abstractThe techniques and samples being employed to find radio galaxies at high redshifts are outlined. Results obtained from the study of high-redshift galaxies, as well as attempts to elucidate this phenomenon are discussed. Several radiooptical correlations have been revealed; these include the so-called alignment effect, which points to the importance of radio jets in triggering bursts of star formation. Apart from serving as important probes of the physical conditions in the universe at different epochs, studies of high-redshift galaxies could help determine if the bulk of galaxy formation occurred in a relatively short span of time at early epochs or whether the process was much more spread out in time, extending to relatively recent epochsen
dc.format.extent1195349 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStar formationen
dc.subjectRadio galaxiesen
dc.titleThe most distant radio galaxiesen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
paper-6.pdf1.17 MBAdobe PDFThumbnail
View/Open


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