Models for X-ray Emission from Radio Quiet AGNs

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dc.creatorHaardt, Francesco
dc.date1996-12-09
dc.date.accessioned2026-07-25T12:53:29Z
dc.descriptionThe current status of understanding of the X-ray emission from Seyfert galaxies involves thermal Comptonization of soft photons by mildrelativistic electrons and positrons. I review observational and theoretical arguments supporting such a view, discussing current models proposed for the structure of the innermost part of the accretion flow: extended coronae, small scale flaring blobs, advection dominated accretion disks and small scale cold cloudlets.
dc.description8 pages, 1 figure.ps. Latex (memsait.sty). To apper in the Proceedings of "Dal Micro al Mega Parsec: Secondo Congresso Nazionale sui Nuclei Galattici Attivi (From Micro to Mega Parsecs: Second Italian National Workshop on Active Galactic Nuclei)"
dc.identifierhttps://arxiv.org/abs/astro-ph/9612082
dc.identifierhttp://arxiv.org/abs/astro-ph/9612082
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/12677
dc.subjectAstrophysics
dc.titleModels for X-ray Emission from Radio Quiet AGNs
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