Two-phase pair corona model for AGN: physical modelling and diagnostics

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dc.creatorPoutanen, Juri
dc.creatorSvensson, Roland
dc.creatorStern, Boris
dc.date1997-01-22
dc.date.accessioned2026-07-07T02:22:47Z
dc.date.available2026-07-07T02:22:47Z
dc.descriptionThe predictions of the two-phase accretion disc-corona models for active galactic nuclei are compared with observations. We discuss the possibility to use X-ray spectral slopes, equivalent widths of the iron line, and the observed flux-spectral index correlation as diagnostics of the X/gamma-ray source compactness and geometry as well as of the cold disc temperature. As an example of the application of the modelling tools, we use XSPEC to fit the broad-band data of Seyfert 1 galaxy, IC4329A, with a theoretical spectrum from a hemisphere-corona.
dc.description5 pages; esa_sp_latex style; 6 postscript figures; Comments to juri@astro.su.se; to appear in the proceeding of the 2nd INTEGRAL Workshop; St.Malo, France, September 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9701168
dc.identifierhttp://arxiv.org/abs/astro-ph/9701168
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11001
dc.subjectAstrophysics
dc.titleTwo-phase pair corona model for AGN: physical modelling and diagnostics
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