Models for X-ray Emission from Radio Quiet AGNs

Simple item page
dc.creatorHaardt, Francesco
dc.date1996-12-09
dc.date.accessioned2026-07-07T02:22:30Z
dc.date.available2026-07-07T02:22:30Z
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.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10897
dc.subjectAstrophysics
dc.titleModels for X-ray Emission from Radio Quiet AGNs
dc.typetext

Files

Collections

arXiv