On the variability and spectral distortion of fluorescent iron lines from black hole accretion discs
A. NiedźwieckiŁódź University, Department of Physics, Pomorska 149/153, 90-236 Łódź, PolandP. T. ŻyckiNicolaus Copernicus Astronomical Centre, Bartycka 18, 00-716 Warsaw, Poland
2008en
ABI
Annotatsiya
Broad iron lines observed from many black hole systems most likely originate from the innermost regions of an accretion disc and their profiles are shaped by gravitational redshift and Doppler shifts. Modelling of the lines observed in
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