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Strong Soft X-ray Emission and High Accretion Rates in Seyfert Galaxies
Published online by Cambridge University Press: 12 April 2016
Abstract
Slim accretion disk models with high accretion rates provide a natural explanation for the strong soft X-ray emission observed in several narrow–line Seyfert 1 galaxies.
- Type
- Part 15. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 812 - 813
- Copyright
- Copyright © Astronomical Society of the Pacific 1997
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