X-ray bright optically quiet galaxies: the case of P3

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dc.creatorComastri, A.
dc.creatorBrusa, M.
dc.creatorCiliegi, P.
dc.creatorMignoli, M.
dc.creatorVignali, C.
dc.creatorSevergnini, P.
dc.creatorMaiolino, R.
dc.creatorFiore, F.
dc.creatorLa Franca, F.
dc.creatorMatt, G.
dc.creatorPerola, G. C.
dc.creatorBaldi, A.
dc.creatorMolendi, S.
dc.date2001-09-07
dc.date.accessioned2026-07-07T01:59:53Z
dc.date.available2026-07-07T01:59:53Z
dc.descriptionRecent X-ray surveys have clearly demonstrated that a population of optically dull, X-ray bright galaxies is emerging at X-ray fluxes of the order of 10-14 erg cm-2 s-1. The nature of these objects is still unknown. We present the results of multiwavelength observations of what can be considered the best studied example: the Chandra source CXOUJ031238.9-765134 optically identified by Fiore et al. (2000) with an apparently normal galaxy at z=0.159 and called ``Fiore P3''.
dc.description6 pages, 4 figures, presented at the meeting: "Issues in unifications of AGNs" Marciana Marina, May 2001; eds. R. Maiolino, A. Marconi and N. Nagar
dc.identifierhttps://arxiv.org/abs/astro-ph/0109117
dc.identifierhttp://arxiv.org/abs/astro-ph/0109117
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3291
dc.subjectAstrophysics
dc.titleX-ray bright optically quiet galaxies: the case of P3
dc.typetext

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