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The Fe Kα Line and Relativistic Effects from Accretion Disks
Published online by Cambridge University Press: 12 April 2016
Abstract
One of the most exciting results from ASCA has been the discovery of relativistic line profiles for iron Kα emission from Seyfert 1 galaxies. Recent results concerning the properties of Fe Kα lines from the inner regions of black-hole accretion disks are reviewed.
- Type
- Part 1. Setting the Scene
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 27 - 37
- Copyright
- Copyright © Astronomical Society of the Pacific 1997