Line Profile Variability in AGNs

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Line Profile Variability in AGNs

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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

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