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A&A 414, 155-161 (2004)
DOI: 10.1051/0004-6361:20031635
The high energy emission line spectrum of NGC 1068
G. Matt1, S. Bianchi1, M. Guainazzi2 and S. Molendi31 Dipartimento di Fisica, Università degli Studi Roma Tre, via della Vasca Navale 84, 00146 Roma, Italy
2 XMM-Newton Science Operation Center/RSSD-ESA, Villafranca del Castillo, Spain
3 IASF-CNR, Via Bassini 15, 20133, Milano, Italy
(Received 21 August 2003 / Accepted 17 October 2003 )
Abstract
We present and discuss the high energy (
E>4 keV) XMM-Newton
spectrum of the Seyfert 2 galaxy, NGC 1068. Possible evidence for flux variability in both
the neutral and ionized reflectors with respect to a BeppoSAX observation taken 3.5 years before is
found. Several Fe and Ni emission lines, from both neutral and highly ionized material, are
detected. The intensity of the iron K
Compton shoulder implies that the
neutral reflector is Compton-thick, likely the visible inner wall of the
cm
-2
absorber. From the equivalent width of the ionized iron lines a column density of a
few
cm
-2 is deduced for the hot ionized reflector. Finally, an iron (nickel)
overabundance, when compared to solar values, of about 2 (4) with respect to lower
Z
elements, is found.
Key words: galaxies: individual: NGC 1068 -- galaxies: Seyfert -- X-rays: galaxies
Offprint request: G. Matt, matt@fis.uniroma3.it
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© ESO 2004
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