Journal
ASTROPHYSICAL JOURNAL
Volume 571, Issue 2, Pages 771-778Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/340016
Keywords
galaxies : active; galaxies : individual (P3); galaxies : nuclei; X-rays : galaxies
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Recent X-ray surveys have clearly demonstrated that a population of optically dull, X-ray bright galaxies is emerging at 2-10 keV fluxes of the order of 10(-14) ergs cm(-2) s(-1). Although they might constitute an important fraction of the sources responsible for the hard X-ray background, their nature is still unknown. With the aim of better understanding the physical mechanisms responsible for the observed properties, we have started an extensive program of multiwavelength follow-up observations of hard X-ray, optically quiet galaxies discovered with XMM-Newton. Here we report the results of what can be considered the first example of this class of objects: CXOU J031238.9-765134, originally discovered by Chandra, and optically identified by Fiore et al. (2000) with an apparently normal early-type galaxy at z = 0.159, usually known as FIORE P3. Analysis of the broadband energy distribution suggests the presence of a heavily obscured active nucleus.
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