arXiv · astro-ph/0612127
The soft X-ray spectrum of PG1211+143
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.
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K. A. Pounds, K. L. Page, J. N. Reeves. 2006-12-05. The soft X-ray spectrum of PG1211+143. https://doi.org/10.1017/s1743921307004796
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