Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2075
Full metadata record
DC FieldValueLanguage
dc.contributor.authorRavindranath, S-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2008-02-28T07:35:51Z-
dc.date.available2008-02-28T07:35:51Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 1, pp. 169 - 170en
dc.identifier.urihttp://hdl.handle.net/2248/2075-
dc.description.abstractWe propose the study of star - forming galaxies at high redshifts with large 10-m class telescopes. Lyman break galaxies serve as the best candidates to probe galaxy formation and evolution. The faintness of these objects (I814 < 24) necessitates the use of large telescopes.en
dc.format.extent205070 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..169Ren
dc.subjectGalaxy formationen
dc.subjectGalaxy evolutionen
dc.subjectLyman break galaxiesen
dc.titleLyman break galaxies at high redshifts (Z > 3) as probes of galaxy formationen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Swara.pdf200.26 kBAdobe PDFThumbnail
View/Open


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