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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