Physics
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...32p&link_type=abstract
XMM-Newton Proposal ID #03009104
Physics
Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Mrk 684, 5C 3.100, 1E 0919+515, Mrk 507, Xmm-Newton Proposal 03009104
Scientific paper
We propose to observe a sample of four Narrow Line Seyfert 1 galaxies with strong Fe II emission (FeNLS1s) for a total allocation time of 115 ks. The goal of this proposal is to test how common is the spectral hard X-ray (E~7-8 keV) absorption feature in FeNLS1s, recently observed in two objects of this class. This feature appears as a clear signature of dense matter outflowing from the nucleus. If our optically-based criterion (i.e. Fe II4570/Hbeta higher than 1.5) would be efficient in selecting objects with deep sharp X-ray edges, the origin of this feature in outflowing clouds would be supported. A frequent occurrence of this spectral drop will therefore provide clues of an intimate link between NLS1s and BAL QSOs phenomena.
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