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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2834
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dc.contributor.authorIshwara-Chandra, C. H-
dc.contributor.authorAnantharamaiah, K. R-
dc.contributor.authorDwarakanath, K. S-
dc.date.accessioned2008-07-23T07:45:48Z-
dc.date.available2008-07-23T07:45:48Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 747 - 748en
dc.identifier.urihttp://hdl.handle.net/2248/2834-
dc.description.abstractWe report the GMRT detection of H I absorption in the high_ redshlft red quasar 30 190 at a redshift of 1.1946. The most interesting result is that the peak of the H I absorption is blueshifted by I'W 250 kms-1 with respect to the optical emission lines. The H I absorption profile indicates the presence of multiple components and the peak: absorption is at 647.728 MHz. The FWHM of this absorption feature is 185 ±7 kms-1and the peak optical depth is 0.012. The corresponding atomic hydrogen column density is 3.98 x 1020 (T8/100K) cm-2•en
dc.format.extent73599 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectGalaxiesen
dc.subjectActive Quasarsen
dc.subjectAbsorption linesen
dc.subjectRadio Linesen
dc.titleGMRT detection of H I absorption in the high-redshift red quasar 3C 190en
dc.typeArticleen
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