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X-rays from Photoionized Accretion Discs
Published online by Cambridge University Press: 19 July 2016
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The presence of iron lines and high energy excesses in the X-ray spectra of Seyfert galaxies has been firmly established by Ginga (e.g. Nandra & Pounds 1993 and references therein). These features are generally interpreted as signatures of the reprocessing of the primary X-rays by matter in the neighbourhood of the central black hole, probably distributed in an accretion disc (Lightman & White 1988, George & Fabian 1991, Matt, Perola & Piro 1991).
- Type
- Poster Contributions: X-Rays and Higher Energies
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- Copyright © Kluwer 1994
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