Results from Recent Deep Simultaneous HST/FUSE/Chandra Campaigns

Details Results from Recent Deep Simultaneous HST/FUSE/Chandra Campaigns Results from Recent Deep Simultaneous HST/FUSE/Chandra Campaigns

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.5005a&link_type=abstract

American Astronomical Society Meeting 204, #50.05; Bulletin of the American Astronomical Society, Vol. 36, p.752

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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

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