The iron 6.4 keV Kα observations and suspicions on the disc-line models.

Details The iron 6.4 keV Kα observations and suspicions on the disc-line models. The iron 6.4 keV Kα observations and suspicions on the disc-line models.

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..254y&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 3, p. 254 - 256

Computer Science

Active Galactic Nuclei: Iron Lines, Active Galactic Nuclei: Radiation Mechanisms

Scientific paper

Data show that, in some AGNs, Seyfert galaxies in particular, the observed iron line is found to be very broad and asymmetric, peaked at 6.4 keV, the position of Kα line of neutral or low-ionized iron, and extended redward to 4 - 5 keV. The generally accepted models - the "disk-line models" - are markedly incompatible with the observed line profiles and intensities.

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