Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S238(2), p. 425-426, 2006
DOI: 10.1017/s1743921307005777
Wiley, Astronomische Nachrichten, 10(327), p. 957-960, 2006
Full text: Unavailable
AbstractSome aspects of power-spectral densities (PSD) of active galactic nuclei are similar to those of galactic black hole X-ray binary systems (McHardy et al. 2005). The signal originates near a black hole and its modulation by general-relativistic effects should be taken into account (Życki & Nedźwiecki 2005). We modified the previous calculations of these effects, assuming a model of spots which occur on the disc surface and decay with a certain lifetime.