FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K lines in AGN

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Autor principal: I. de La Calle
Formato: Artículo científico
Lenguaje:en
Publicado: Universidad Nacional Autónoma de México 2008
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author I. de La Calle
author_facet I. de La Calle
contents FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K lines in AGN I. de La Calle M. Dovciak A. L. Longinotti S. Bianchi M. Guainazzi Física, Astronomía y Matemáticas line: profiles rays: galaxies Galaxies: active The properties of the relativistically broadened Fe Kα line emitted in Active Galactic Nuclei (AGN) are stilldebated among the AGN community. Recent works seem to exclude that the broad Fe line is a common featureof AGN. The analysis of a large sample composed by 157 XMM-Newton archival observations of radio quietAGN is presented here. This ongoing project is a development of the work reported in Guainazzi et al. (2006). 2008 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57103223 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.32
format Artículo científico
id redalyc_57103223
institution Redalyc
language en
publishDate 2008
publisher Universidad Nacional Autónoma de México
spellingShingle FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K lines in AGN
I. de La Calle
Física, Astronomía y Matemáticas
line: profiles
rays: galaxies
Galaxies: active
FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K lines in AGN I. de La Calle M. Dovciak A. L. Longinotti S. Bianchi M. Guainazzi Física, Astronomía y Matemáticas line: profiles rays: galaxies Galaxies: active The properties of the relativistically broadened Fe Kα line emitted in Active Galactic Nuclei (AGN) are stilldebated among the AGN community. Recent works seem to exclude that the broad Fe line is a common featureof AGN. The analysis of a large sample composed by 157 XMM-Newton archival observations of radio quietAGN is presented here. This ongoing project is a development of the work reported in Guainazzi et al. (2006). 2008 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57103223 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.32
title FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K lines in AGN
topic Física, Astronomía y Matemáticas
line: profiles
rays: galaxies
Galaxies: active
url https://www.redalyc.org/articulo.oa?id=57103223