The soft X-ray spectrum of PG1211+143
arXiv:astro-ph/0612127 · doi:10.1017/S1743921307004796
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.
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