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N. Arav (University of Colorado)
We discuss the connection between the UV and X-ray manifestation of AGN outflows based on recent deep HST/FUSE/Chandra simultaneous campaigns. Based on their phenomenological similarity, the UV and X-ray troughs seem to arise from the same physical outflow. Therefore, we argue that the current methods used to extract column densities from X-ray troughs are inadequate, and suggest several ways to improve the situation
The author(s) of this abstract have provided an email address for comments about the abstract: arav@colorado.edu
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Bulletin of the American Astronomical Society, 36 #2
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