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GMRT detection of HI absorption in the high-redshift red quasar 3C 190

dc.contributor.authorIshwara-Chandra, C H
dc.contributor.authorAnantharamaiah, K R
dc.contributor.authorDwarakanath, K S
dc.date.accessioned2006-06-12T10:49:09Z
dc.date.available2006-06-12T10:49:09Z
dc.date.issued2002
dc.descriptionPresented at the 21st meeting of the Astronomical Society of India, Pune, 2002.en
dc.description.abstractWe report the GMRT detection of H I absorption in the high- redshift red quasar 3C 190 at a redshift of 1.1946. The most interesting result is that the peak of the H I absorption is blue shifted by - 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 10^20 (T,/100K) cm-2.en
dc.format.extent397176 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationBulletin of the Astronomical Society of India, 2002, Vol.30, p747-748en
dc.identifier.issn0304-9523
dc.identifier.urihttp://hdl.handle.net/2289/1358
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.rights(2002) by the Astronomical Society of India.en
dc.subjectGalaxiesen
dc.subjectactive – quasarsen
dc.subjectabsorption lines - radio lies: galaxiesen
dc.titleGMRT detection of HI absorption in the high-redshift red quasar 3C 190en
dc.typeArticleen

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