FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K alpha lines in AGN

Details FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K alpha lines in AGN FERO (Finding Extreme Relativistic Objects): statistics of relativistic broad Fe K alpha lines in AGN

2007-09-20

arxiv.org/abs/0709.3268v2

Astronomy and Astrophysics

Astrophysics

Proceeding of "The nuclear region, host galaxy and environment of active galaxies", symposium for the 60th birthday of Deborah

Scientific paper

The properties of the relativistically broadened Fe K alpha line emitted in Active Galactic Nuclei (AGN) are still debated among the AGN community. Recent works seem to exclude that the broad Fe line is a common feature of AGN. The analysis of a large sample composed by 157 XMM-Newton archival observations of radio quiet AGN is presented here. This ongoing project is a development of the work reported in Guainazzi et al. 2006.

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