dc.contributor.author |
Narasimha, D |
|
dc.contributor.author |
Srianand, R |
|
dc.date.accessioned |
2008-03-15T11:06:45Z |
|
dc.date.available |
2008-03-15T11:06:45Z |
|
dc.date.issued |
2000 |
|
dc.identifier.citation |
BASI, Vol. 28, No. 2, pp. 395 - 396 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2159 |
|
dc.description.abstract |
Using 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.extent |
209696 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2000BASI...28..395N |
en |
dc.subject |
AGN: broad absorption lines |
en |
dc.subject |
Gravitational lensing |
en |
dc.title |
Study of quasar broad emission region from spectroscopy of multiple images |
en |
dc.type |
Article |
en |