dc.contributor.author |
Shastri, P |
|
dc.date.accessioned |
2008-03-07T09:01:57Z |
|
dc.date.available |
2008-03-07T09:01:57Z |
|
dc.date.issued |
2007-10 |
|
dc.identifier.citation |
Astronomical Society of the Pacific Conference Series, Vol. 373, pp. 435 - 438 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2143 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
With the realization that orientation plays a dominant role in the appearance of active galaxies, much of AGN research has been worked into the operating framework of the �unified scheme,� wherein active galaxies are broadly classified into three physically distinct classes: radio-quiet, radio-loud Fanaroff-Riley I and radio-loud Fanaroff-Riley II, with the appearance in each of the three cases being dominated by orientation alone. The following is a brief summary of the current understanding on the domain of validity of the scheme. |
en |
dc.format.extent |
130201 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of the Pacific |
en |
dc.relation.uri |
http://aspbooks.org/custom/publications/paper/373-0435.html |
en |
dc.subject |
Active Galaxies |
en |
dc.title |
Different Angles on Active Galaxies: Where are We with Regard to Unification? |
en |
dc.type |
Article |
en |