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A&A 410, 471-479 (2003)
DOI: 10.1051/0004-6361:20031124
The complex FeK line of the Narrow-Line Seyfert 1 galaxy IRAS 13349+2438
A. L. Longinotti1, 2, M. Cappi2, K. Nandra1, M. Dadina2 and S. Pellegrini31 Astrophysics Group, Imperial College of Science, Technology and Medicine, Prince Consort Rd. SW7 2AZ, London, UK
2 Istituto IASF-CNR, Sezione di Bologna Via Gobetti 101, 40129 Bologna, Italy
3 Universita' degli studi di Bologna, Dipartimento di Astronomia, via Ranzani 1, 40127 Bologna, Italy
(Received 7 April 2003 / Accepted 24 July 2003)
Abstract
The observation of the Narrow-Line Seyfert 1 galaxy IRAS 13349+2438 performed
by XMM-Newton European Photon Imaging Camera between 0.3-10 keV, is presented here.
The broadband spectrum of the source is dominated at low energies
(
keV) by a strong excess of emission and by complex
emission/absorption features between ~5.5-8.0 keV.
The soft X-ray spectrum is consistent with ionized absorption found by the Reflection Grating Spectrometer (Sako et al. 2001a).
We focus on the 2-10 keV spectrum which shows
clear evidence for a broad, complex FeK
line, previously
unseen by ASCA, and for an Fe K-shell edge detected at ~7.3-7.4 keV
(rest-frame).
The presence of this edge could be explained by either
partial covering or ionized/relativistic reflection models, with the
latter being preferred and with a resulting power law slope of
.
The line profile is complex, with a broad bump between ~5.5-6.5 keV and
a narrow emission line at ~7 keV, separated by a sharp drop at ~6.8 keV.
This profile is compatible with two possible scenarios:
i) a broad, ionized and gravitationally redshifted Laor diskline plus a narrow and ionized
emission line; ii) a broad, ionized and single Schwarzschild (double-peaked) diskline with a
superimposed narrow absorption line.
Key words: X-rays: galaxies -- galaxies: Seyfert -- galaxies: individual: IRAS 13349+2438
Offprint request: A. L. Longinotti, all@imperial.ac.uk
SIMBAD Objects
© ESO 2003
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