I would like to thank my primary collaborators Jeff Linsky, Hans Müller, Gary Zank, and Vlad Izmodenov for their contributions to the astrospheric Ly research. I would also like to thank David McComas and Rosine Lallement for providing figures for this article, and Priscilla Frisch for fruitful discussions. Support for this work was provided by NASA through grants NAG5-9041 and NNG05GD69G to the University of Colorado, and through grant number AR-09957 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS5-26555. Extensive use of NASA’s Astrophysics Data System Bibliographic Services has been made in the preparation of this article.
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