Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-02-27
Astronomy and Astrophysics
Astrophysics
11 pages (LaTeX), 7 figures (EPS); PASJ accepted
Scientific paper
We have explored spectral line profiles due to spiral patterns in accretion discs around black holes. A parametrization was employed for the shape and emissivity of spiral waves, which can be produced by non-axisymmetric perturbations affecting the disc density and ionization structure. The effects of the light-travel time, energy shift, and gravitational focusing near to a rotating black hole were taken into account. A high-resolution ray-tracing code was used to follow the time variations of the synthetic line profile. A variety of expected spectral features were examined and the scheme applied to a broad iron line observed in MCG-6-30-15.
Karas Vladimir
Martocchia Andrea
Subr Ladislav
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