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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
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
- 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
References
Nandra, K., O'Neill, P. M., George, I. M., & Reeves, J. N. 2007, M.N.R.A.S., 382, 194CrossRefGoogle Scholar
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