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Reprocessing Models and the ASCA Spectrum of Mkn 290

Published online by Cambridge University Press:  12 April 2016

T. J. Turner ,
I. M. George ,
T. Kallman ,
T. Yaqoob  and
P.T. Życki
T. J. Turner
Affiliation:
Laboratory for High Energy Astrophysics, Code 660, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
I. M. George
Affiliation:
Laboratory for High Energy Astrophysics, Code 660, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
T. Kallman
Affiliation:
Laboratory for High Energy Astrophysics, Code 660, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
T. Yaqoob
Affiliation:
Laboratory for High Energy Astrophysics, Code 660, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
P.T. Życki
Affiliation:
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716, Warsaw, Poland

Abstract

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We describe a warm absorber/emitter model that is used to model the complex X-ray spectrum of Mkn 290. The best fit to the data also includes a contribution from an ionized reflector.

Type
V. Emission Lines, Absorption Lines, the Continuum, and their Relationships
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 244 - 245
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Turner, T.J., George, I.M., Kallman, T., Yaqoob, T., & Życki, P.T. 1996, ApJ, 472, in press.Google Scholar