FUSE Cycle 7 Guest Investigator observing programs, sorted by the last name of the Principal Investigator. 16 January 2006 PgmID PI Last Name Pgm Type PI Institution Observing Program Title ----------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- G023 Ayres Standard University of Colorado High-Declination Late-Type Supergiants in the Mass Range 5-7 Suns G059 Blair Standard Johns Hopkins University The Enigmatic Magellanic Cloud Supernova Remnant N63A G931 Blair Survey/Supplementary Johns Hopkins University FUSE Survey of Magellanic Cloud Supernova Remnants Continued G020 Bowen Standard Princeton University A Search for Hot Baryons in the Halos of Nearby Galaxies G701 Brown Survey/Supplementary University of Colorado Stellar Activity in the 30 Myr old Tucana-Horologium Association G061 Chayer Standard Johns Hopkins University FUSE Observations of Hot Subdwarf B Stars G917 Crenshaw Survey/Supplementary Georgia State University Variable Absorption in the Seyfert Galaxy NGC 3516 G053 Danforth Standard University of Colorado O VI and C III Emission from LMC Superbubble N70 G081 DeWarf Standard Villanova University Deep Quiescent Magnetic Activity State of alpha Cen A G073 Dixon Standard Johns Hopkins University FUSE Observations of the UV-Bright Star in 47 Tucanae G057 Dunne Standard University of Illinois O VI Emission from the Interface Layers in the Superbubbles DEM152 and DEM192 G048 Dupree Standard Smithsonian Astrophysical ObservaA Test of Wind Dynamics in Accreting Young Stars G921 Dupuis Survey/Supplementary Canadian Space Agency Metals and Quasi-Molecular Satellites in Cooler DA White Dwarfs G058 Espey Standard Trinity College Belfast Understand Mass-loss in Cool Giants: the Wind of SY Mus G932 Friedman Survey/Supplementary Space Telescope Science InstituteProbing Small-Scale ISM Variations with Multi-Epoch FUSE Observations G035 Gaetz Standard Smithsonian Astrophysical ObservaDynamics of a Young, O-Rich Supernova Remnant in the SMC G067 Ghavamian Standard Johns Hopkins University The Nebular Shell Around the Ultraluminous X-ray Source Ho IX X-1 -- Supershell or Hypernova Remnant? G027 Giroux Standard East Tennessee State Univ. An Abundance Study of the Magellanic Stream G925 Godon Survey/Supplementary Villanova University FUSE Survey of Dwarf Novae: basic characteristics of the WD and accretion disk G936 Gruendl Survey/Supplementary University of Illinois Hot Gas in the Starburst Carina Nebula G060 Guinan Standard Villanova University FUV Observations of the Old High Velocity dM1 Star SZ UMa G006 Gull Standard Goddard Space Flight Center Separating Binary Orbital Variations in Eta Car from Secular Changes G933 Hebrard Survey/Supplementary Institut d'Astrophysique de ParisSurveying the sight lines of subdwarfs beyond the Local Bubble G007 Henry Standard Johns Hopkins University Diffuse UV Background G038 Herald Standard Johns Hopkins University Investigating the Neon Abundance of LMC WO stars G039 Herald Standard Johns Hopkins University Wolf-Rayet Stars in Environments of Different Metallicity G050 Howk Standard University of Notre Dame Far-Ultraviolet Study of the Magellanic Bridge G051 Howk Standard University of Notre Dame Tidal Debris and Halos about the Magellanic Clouds G013 Iping TOO Catholic University of America Probing the Halo and ISM of Low-Redshift Galaxies with Young Supernovae G025 Iping Standard Catholic University of America FUV Study of the Extreme Wolf-Rayet Binary CQ Cephei G927 Iping Survey/Supplementary Catholic University of America Mass Loss Processes in LBVs and Late-Type WR Stars G017 Jenkins Standard Princeton University Why is Some H I in Interstellar Atomic Clouds so Extraordinarily Cold? G018 Knauth Standard Northwestern University The Enigma of the Interstellar N2 Abundance G029 Leighly Standard University of Oklahoma Tropical Storm to Hurricane: The Emergence of a BAL Wind G036 Moffat Standard Universite de Montreal Does Metallicity Affect Clumping in Hot-Star Winds? G003 Oliveira Standard Johns Hopkins University H I, D I and other abundances along three extended sightlines G063 Penny Standard College of Charleston The Effect of Metallicity of the Rotation Rates of Massive Stars G076 Peters Standard University of Southern CaliforniaAbundances of C and N in the Be Star NGC330-B12 in the SMC G923 Peters Survey/Supplementary University of Southern CaliforniaMass Transfer in the Active Interacting Binary U~Cephei G924 Peters Survey/Supplementary University of Southern CaliforniaA FUSE Survey of Be Stars in Galactic Clusters G015 Redfield Standard University of Texas Austin Variations in the Ionization Structure within the LIC and Neighboring Clouds G052 Sankrit Standard Johns Hopkins University O VI Emission from Conductive Interfaces in the LISM G938 Sankrit Survey/Supplementary Johns Hopkins University Survey of O VI Emission towards Nearby White Dwarfs G044 Shull Standard University of Colorado Detecting the Elusive Hot Baryons in O~VI G021 Skillman Standard University of Minnesota The True Chemical Abundances of Dwarf Galaxies G712 Thilker Survey/Supplementary Johns Hopkins University Probing Extranuclear Star-Forming Regions from SINGS G713 Thilker Survey/Supplementary Johns Hopkins University FUSE Survey Observations of UV-Bright Stellar Complexes G010 Wakker Standard University of Wisconsin Studying the Warm-Hot Ionized Medium in Groups of Galaxies G062 Wesemael Standard Universite de Montreal Trace Elements at the Photospheres of DB White Dwarfs