IIA Institutional Repository

The most distant radio galaxies

Show simple item record

dc.contributor.author Kapahi, V. K
dc.date.accessioned 2007-03-21T06:45:58Z
dc.date.available 2007-03-21T06:45:58Z
dc.date.issued 1992
dc.identifier.citation BASI, Vol. 20, pp 49-60 en
dc.identifier.uri http://hdl.handle.net/2248/1458
dc.description.abstract The 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 epochs en
dc.format.extent 1195349 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.subject Star formation en
dc.subject Radio galaxies en
dc.title The most distant radio galaxies en
dc.type Article en


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account