Add to ORKGWe calculate the iron fluorescent Kw. line intensity from an accretion disc orbiting around a maximally rotating black hole and illuminated by an X-ray source located on the hole rotation axis. We find that the line intensity can be much greater than that obtained from illuminated accretion discs around static black holes. This provides a possible explanation for the large iron line equivalent widths observed in some Seyfert 1 galaxies
The observed iron K-alpha fluorescence lines in Seyfert-1 galaxies provide strong evidence for an ac...
Ginga observations of several bright Seyfert 1 galaxies have recently revealed the presence in their...
Recent X-ray spectroscopy made with ASCA have shown broad, skewed iron line emission from Seyfert-1 ...
We calculate the iron fluorescent Kw. line intensity from an accretion disc orbiting around a maxima...
The intensity and profile of the iron K-alpha fluorescence line from a flat, optically thick accreti...
The fluorescent iron K$\alpha$ emission line profile provides an excellentprobe of the innermost reg...
The observed iron K{alpha} fluorescence lines in Seyfert I galaxies provide strong evidence for an a...
The properties of the iron Kalpha line emitted by an accretion disc illuminated by an external X-ray...
X-ray reflection spectra from photoionized accretion discs in active galaxies are presented for a wi...
Context. Spectroscopy of X-ray emission lines emitted from accretion discs around supermassive black...
Previous calculations of Fe K-alpha line profiles are based on axisymmetric emissivity laws. In this...
Broad iron lines are expected, and observed, to be a widespread feature in bright AGN. Still unclear...
In this paper we present a fully relativistic approach to modelling both the continuum emission and ...
International audienceSince the 1995 discovery of the broad iron K-line emission from the Seyfert ga...
Context. We present angle-dependent, broad-band intensity spectra from accretion disks around black ...
The observed iron K-alpha fluorescence lines in Seyfert-1 galaxies provide strong evidence for an ac...
Ginga observations of several bright Seyfert 1 galaxies have recently revealed the presence in their...
Recent X-ray spectroscopy made with ASCA have shown broad, skewed iron line emission from Seyfert-1 ...
We calculate the iron fluorescent Kw. line intensity from an accretion disc orbiting around a maxima...
The intensity and profile of the iron K-alpha fluorescence line from a flat, optically thick accreti...
The fluorescent iron K$\alpha$ emission line profile provides an excellentprobe of the innermost reg...
The observed iron K{alpha} fluorescence lines in Seyfert I galaxies provide strong evidence for an a...
The properties of the iron Kalpha line emitted by an accretion disc illuminated by an external X-ray...
X-ray reflection spectra from photoionized accretion discs in active galaxies are presented for a wi...
Context. Spectroscopy of X-ray emission lines emitted from accretion discs around supermassive black...
Previous calculations of Fe K-alpha line profiles are based on axisymmetric emissivity laws. In this...
Broad iron lines are expected, and observed, to be a widespread feature in bright AGN. Still unclear...
In this paper we present a fully relativistic approach to modelling both the continuum emission and ...
International audienceSince the 1995 discovery of the broad iron K-line emission from the Seyfert ga...
Context. We present angle-dependent, broad-band intensity spectra from accretion disks around black ...
The observed iron K-alpha fluorescence lines in Seyfert-1 galaxies provide strong evidence for an ac...
Ginga observations of several bright Seyfert 1 galaxies have recently revealed the presence in their...
Recent X-ray spectroscopy made with ASCA have shown broad, skewed iron line emission from Seyfert-1 ...