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Modeling the UV-X-spetrum

dc.contributor.authorGoosmann, René W.
dc.date.accessioned2010-10-12T18:25:32Z
dc.date.available2010-10-12T18:25:32Z
dc.date.issued2006
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-30FD-E
dc.description.abstractWith the last generation of X-ray satellites, such as XMM-Newton and Chandra, our knowledge about the X-ray properties of Active Galactic Nuclei (AGN) has greatly improved. Detailed spectroscopy and long-term observations of hundreds of kilo-seconds have provided new insights into the mechanisms of X-ray production, its modification by intervening matter, and X-ray variability. In this thesis I present radiative transfer modeling of AGN in the Far-UV and X-ray range. The modeling considers several aspects of the observed X-ray properties: the Compton reflection/reprocessed component, X-ray variability and flares, and the effects of the warm absorber. For the X-ray reprocessing, I investigate in detail the magnetic flare model assuming solar-like magnetic reconnections above the accretion disk
dc.format.extent151 S.
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherUniv. Hamburg
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc523
dc.subject.gokTEG 440
dc.subject.gokTBK 000
dc.titleAccretion and emission close to supermassive black holes in quasars and AGN
dc.title.alternativeModeling the UV-X-spetrum
dc.typemonograph
dc.subject.gokverbalSchwarze Löcher {Astronomie: Kosmogonie}
dc.subject.gokverbalHochenergieastronomie
dc.identifier.doi10.23689/fidgeo-117
dc.identifier.ppn516227033
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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