Abstract
Abstract : We report on the results of 3-4 micrometers spectroscopy of the ultraluminous infrared galaxy (ULIRG) UGC 5101. It has a cool far-infrared color and a LINER-type optical spectrum and so, based on a view gaining some currency, would be regarded as dominated by star formation. However, we find that it has strong 3.4 micrometers carbonaceous dust absorption, low equivalent width 3.3 micrometers polycyclic aromatic hydrocarbon (PAH) emission, and a small 3.3 micrometers PAH to far-infrared luminosity ratio. This favors an alternative scenario, in which an energetically dominant active galactic nucleus (AGN) is present behind obscuring dust. The AGN is plausibly obscured along all lines of sight (a AGN) rather than merely obscured along our particular line of sight. Such buried AGNs have previously been found in thermal infrared studies of the ULIRGs IRAS 08572 3915 and IRAS F00183-7111, both classified optically as LINERs. We argue that buried AGNs can produce LINER-type optical spectra and that at least some fraction of LINER-type ULIRGs are predominantly powered by buried AGNs.
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