Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2159
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dc.contributor.authorNarasimha, D-
dc.contributor.authorSrianand, R-
dc.date.accessioned2008-03-15T11:06:45Z-
dc.date.available2008-03-15T11:06:45Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 395 - 396en
dc.identifier.urihttp://hdl.handle.net/2248/2159-
dc.description.abstractUsing the high resolution radio observations and analysis of the broad emission lines as well as continum in the optical spectra of the multiple images of quasars, we provide a method to probe the structure and dynamics of the broad emission region of AGNs. From the study of the system 1422+231 we establish that the optical and radio emission of the source originate from two different regions.en
dc.format.extent209696 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..395Nen
dc.subjectAGN: broad absorption linesen
dc.subjectGravitational lensingen
dc.titleStudy of quasar broad emission region from spectroscopy of multiple imagesen
dc.typeArticleen
Appears in Collections:BASI Publications

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