Published in

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

DOI: 10.1002/asna.200610671

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Power spectra from spotted accretion discs

Journal article published in 2006 by Tomáš Pecháček, Michal Dovčiak ORCID, Vladimír Karas
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

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Data provided by SHERPA/RoMEO

Abstract

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.

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