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Multiwavelength analysis as a probe of accretion and radiative processes in LINERs

Published online by Cambridge University Press:  21 February 2013

George Younes  and
Delphine Porquet
George Younes
Affiliation:
NSSTC, 320 Sparkman Drive, Huntsville, AL 35805, USA email: gyounes@usra.edu
Delphine Porquet
Affiliation:
Observatoire Astronomique de Strasbourg, CNRS, UMR7550, 11 rue de l'Universit, 67000, Strasbourg, France email: delphine.porquet@astro.unistra.fr
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Abstract

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We study the multiwavelength properties of an optically selected sample of Low Ionization Nuclear Emission-line Regions (LINERs), in an attempt to determine the accretion mechanism powering their central engine. We show how their X-ray spectral characteristics, and their spectral energy distribution compare to luminous AGN, and briefly discuss their connection to their less massive counter-parts galactic black-hole X-ray binaries.

Keywords

AGNLINERsaccretionaccretion disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 355 - 356
Copyright
Copyright © International Astronomical Union 2013

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