Multiwavelength analysis as a probe of accretion and radiative processes   in LINERs
  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. 
George Younes (1), Delphine Porquet (2) ((1) USRA/NASA/MSFC, (2)   Observatoire de Strasbourg, France)
astro-ph.HE astro-ph.GA