Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004head....8.0702l&link_type=abstract
American Astronomical Society, HEAD meeting #8, #07.02; Bulletin of the American Astronomical Society, Vol. 36, p.916
Astronomy and Astrophysics
Astronomy
Scientific paper
The study of Fe K lines in AGNs has achieved a remarkable improvement since XMM-Newton data have been available. Many insights on the Fe K lines properties and its relation to the accretion disk structure have been investigated with the aid of the high signal-to-noise spectra provided by this satellite. In this regard, the line emission can be studied more precisely for high luminosity objects than previously done by ASCA, providing a potential tool to understand the links between black hole driving parameters and hard X-ray spectra. Here a study of a sample of XMM-Newton quasars is presented including some new results on individual objects.
Lia Longinotti Anna
Nandra Kirpal
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