The recent X-ray history of NGC 5506
arXiv:astro-ph/0302349 · doi:10.1051/0004-6361:20030210
Abstract
We present a detailed discussion of the spectral and spatial components of NGC 5506, based on XMM-Newton, Chandra and BeppoSAX observations. The overall picture consists of a nucleus absorbed by cold gas with column density of cm and surrounded by a Compton-thick torus, whose existence is inferred by a cold reflection component and an iron K line. On a much larger scale, a photoionized gas extended on pc reprocesses the nuclear radiation, producing a soft excess and ionized iron lines. Noteworthy, we find no evidence for the presence of the accretion disc.
arXiv comment9 pages, 9 figures, accepted for publication in A&A
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