XMM-Newton Detection of a Compton-thick AGN in the 1-Jy ULIRG/LINER F04103-2838
arXiv:0711.0002 · doi:10.1086/524926
Abstract
We report on the detection of Fe Kalpha emission in F041032838, an ultraluminous infrared galaxy (ULIRG; log[L/L] 12) that is optically classified as a LINER. Previous {\it Chandra} observations suggested the presence of both a starburst and an AGN in this source. A deeper (20 ksec) {\it XMM-Newton} spectrum reveals an Fe Kalpha line at rest frame energy 6.4 keV, consistent with cold neutral iron. The best-fit spectral model indicates the Fe Kalpha line has an equivalent width of 1.6 keV. The hard X-ray emission is dominated by a Compton-thick AGN with intrinsic 0.2--10 keV luminosity ergs s, while the soft X-ray emission is from 0.1 keV gas attributed to the starburst. The X-ray spectrum of this source bears a striking resemblance to that of the archetypal luminous infrared galaxy NGC 6240 despite differences in merger state and infrared properties.
arXiv comment23 pre-print pages including 5 figures and 1 table. Accepted by ApJ
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