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The soft X-ray spectrum of PG1211+143

Published online by Cambridge University Press:  01 August 2006

K. A. Pounds ,
K. L. Page  and
J. N. Reeves
K. A. Pounds
Affiliation:
Department of Physics and Astronomy, University of Leicester, UK
K. L. Page
Affiliation:
Department of Physics and Astronomy, University of Leicester, UK
J. N. Reeves
Affiliation:
NASA Goddard Space Flight Center, Code 663, Greenbelt, MD 20771, USA
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Abstract

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The narrow line QSO PG1211+143 has been a focus of recent attempts to understand the soft excess in AGN, while the 2001 XMM-Newton observation of this luminous AGN also provided evidence for a massive and energetic outflow. Here we consider a physical link between the energetic outflow and the variable soft excess.

Keywords

Galaxies: active – galaxies: nuclei
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 105 - 110
Copyright
Copyright © International Astronomical Union 2007

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