The Distances and Origins of the High Velocity Hydrogen     Clouds
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Drs. Antoinette and Lennox Cowie at the University of Hawaii will               use observations of interstellar spectral lines to determine the                distances to high velocity clouds of neutral atomic hydrogen gas.                                                                                               Approximately 10 percent of the Galactic sky is covered by high                 velocity clouds of neutral atomic hydrogen, but their origin and                location has remained elusive for twenty years.  No matter what                 their origin, they are potentially an extremely interesting                     phenomenon which may be important to our understanding of galaxy                evolution and the energy and mass balance of the interstellar                   medium.  The missing key to the high velocity clouds is a                       knowledge of their distances.  The Cowies' project is aimed at                  determining those distances.
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