On the role of relativistic effects in X-ray variability of AGN

dc.creatorZycki, P. T.
dc.creatorNiedzwiecki, A.
dc.date2006-12-20
dc.date.accessioned2026-07-07T07:40:16Z
dc.date.available2026-07-07T07:40:16Z
dc.descriptionSpecial relativistic and strong gravity effects are clearly seen in X-ray energy spectra from AGN. Most important here are the broad profiles of the Fe Kalpha line observed in a large fraction of sources. These indicate that X-ray generation and reprocessing takes place very close to the central black hole. Here we explore consequences of such effects on X-ray variability. We perform computations of a possible quasi-periodic signal from a Keplerian motion of primary X-ray source. We also study in some details the light-bending model of variability of the X-ray reprocessed component, extending previous work on the subject.
dc.descriptionConference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP). 4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0612597
dc.identifierhttp://arxiv.org/abs/astro-ph/0612597
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121724
dc.subjectAstrophysics
dc.titleOn the role of relativistic effects in X-ray variability of AGN
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