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I. George (JCA, UMBC & NASA/GSFC)
Over the past 3 years we have been provided with greatly enhanced observational capabilities and a wealth of new data. However, in the study of Type I AGN, these new observations have raised a number of important issues which are not yet fully understood, controversial, or both. I will give a brief review of several issues which have arisen from high-resolution spectroscopy, concentrating on studies of the "warm-absorber" and of the Fe K-line. I will also discuss the prospects for further progress in the next few years. This work is funded by NASA.
If you would like more information about this abstract, please follow the link to http://www.jca.umbc.edu/~george/html/science/gnt/gnt.shtml. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: ian.george@umbc.edu
Bulletin of the American Astronomical Society,
35#2
© 2003. The American Astronomical Soceity.