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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

Ewa Szuszkiewicz
Ewa Szuszkiewicz*
Affiliation:
Astronomy Group, Department of Physics and Astronomy, University of Leicester, University Road, Leicester, LEI 7RH, England

Abstract

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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

References

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