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R.E. Griffiths, A. Ptak (Carnegie Mellon University)
We present observations of NGC4151 using XMM-Newton, with results in the following areas:
(i) complex iron-line emission, interpreted in terms of the accretion disk and strong gravitational effects near the central black hole
(ii) a low-energy X-ray spectrum containing a strong oxygen line
(iii) the ultraviolet image obtained using the XMM Optical Monitor.
Variability of the X-ray spectrum and line emission has been studied during the 70Ks observation.