| dc.contributor.author |
Kollatschny, Wolfram |
|
| dc.contributor.editor |
Popović, Luka Č. |
|
| dc.date.accessioned |
2011-01-10T11:30:54Z |
|
| dc.date.available |
2011-01-10T11:30:54Z |
|
| dc.date.issued |
2007 |
|
| dc.identifier.isbn |
978-86-80019-17-8 |
en_US |
| dc.identifier.uri |
http://hdl.handle.net/123456789/1457 |
|
| dc.description.provenance |
Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-10T11:30:54Z
No. of bitstreams: 1
I09.pdf: 3287068 bytes, checksum: d0dca60cc07e668428aa8d345f8dffda (MD5) |
en |
| dc.description.provenance |
Made available in DSpace on 2011-01-10T11:30:54Z (GMT). No. of bitstreams: 1
I09.pdf: 3287068 bytes, checksum: d0dca60cc07e668428aa8d345f8dffda (MD5)
Previous issue date: 2007 |
en |
| dc.language.iso |
en |
en_US |
| dc.publisher |
Nenad Milovanović & Milan S. Dimitrijević, Astronomical Observatory, Belgrade |
en_US |
| dc.title |
Line Profile Variability in AGNs |
en_US |
| mf.subject.keywords |
I will review some key aspects of the central line emitting region in AGN. Continuum and
emission line variability provides a powerful tool to map the structure of the central broad
line region (BLR). Observed delays of the emission lines of the order of days to weeks
probe regions only microarcseconds away from the nucleus. I will discuss different
methods to derive the central mass of the supermassive black holes in AGN. Finally, the
2D-reverberation mapping method applied to variable line profiles gives us information on
geometry and velocity in the innermost BLR. |
en_US |
| mf.document.pages |
38 |
en_US |
| mf.contributor.editor-in-chief |
Dimitrijević, S. Milan |
|