The soft X-ray spectrum of PG1211+143
Astrophysics
2009-11-11 v1
Abstract
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
Cite
@article{arxiv.astro-ph/0612127,
title = {The soft X-ray spectrum of PG1211+143},
author = {K. A. Pounds and K. L. Page and J. N. Reeves},
journal= {arXiv preprint arXiv:astro-ph/0612127},
year = {2009}
}
Comments
to be published in 'Black Holes: from Stars to Galaxies - across the Range of Masses. Proceedings IAU Symposium No. 238, 2006. V.Karas and G.Matt, eds