This file contains a listing, sorted by proposal ID number (PID), of all non-solar system programs approved for cycle 3. This listing also contains the name of the Principal Investigator (PI), his/her institution, and the title of the proposal. PID PI Institution Title ------------------------------------------------------------------------------------------------------------------------------------- C001 Welsh University of California, Berkeley A far UV study of high velocity atomic and molecular gas associated with the evolved Shajn 147 SNR C002 Massey Lowell Observatory FUSE Observations of LMC and SMC O3-4 Stars - the Physical Parameters of the Hottest Stars C007 Dinerstein University of Texas, Austin Radiative Cascade Emission from Molecular and Ionized Gas in Planetary Nebulae C008 Hoard Cerro Tololo Inter-American Observatory Mass Transfer in the Interacting Binary White Dwarf AM Canum Venaticorum C010 Wood San Diego State University Flares, Magnetic Reconnections and Accretion Disk Viscosity C011 Evans Smithsonian Astrophysical Observatory The Mass of the Classical Cepheid S Mus C017 Walter SUNY Stony Brook The early evolution of the circumstellar environment of solar-like stars C018 Walter SUNY Stony Brook The Peculiar B Star HD 28867E C019 Brandt The Pennsylvania State University Monitoring the Variable UV Absorption in NGC4051 with FUSE C020 Dreizler Universitat Tubingen Time resolved spectroscopy of the sdB variable PG1605+072 C022 Harper University of Colorado at Boulder Chromospheric Activity in Population II Giants C023 Harper University of Colorado Evolved Late-Type Star FUV Spectra Mass Loss & Fluorescence C026 Lanz University of Maryland FUSE Observations of Key DBA and DAB White Dwarfs C027 Ferland University of Kentucky Orions Veil, Magnetic Bomb or Gossamer Sheet C029 Raymond CfA A Face-On Collisionless Shock in the Cygnus Loop C030 Sabra University of Florida The Physics of AAL Quasars C034 Tovmassian Instituto de Astronomia Probing The Most Oxygen-Poor Halo Planetary Nebula C036 Benjamin University of Wisconsin-Madison Molecular Gas In The Disk-Halo Interface C037 Benjamin University of Wisconsin A search for OVI emission from high-velocity clouds C038 Simon University of Hawaii Seeing Double - Do the X-Ray Luminous Early A Stars Have Active Binary Companions C041 Szkody University of Washington A Study of the Inner Disk and Hot White Dwarf in Novalikes Above the Period Gap C043 Morrison The University of Toledo The Stellar Wind of Deneb (Alpha Cygni, A2 Ia) C046 Provencal University of Delaware The Temperature Scale and Chemical Composition of DB White Dwarfs C048 Heckman Johns Hopkins University A UV Spectroscopic Survey of Starburst Galaxies C049 Pellerin Universite Laval Young Stellar Populations in Nuclear Starbursts and AGNs C050 Burleigh University of Leicester The white dwarf companions of late-type B stars C051 Blair Johns Hopkins University Kinematics and Composition of O-rich Material in Puppis A C052 Blair Johns Hopkins University Absorption-Emission Line Study of the Northeast Cygnus Loop C053 Barstow University of Leicester The mass distribution of white dwarfs in cataclysmic variables C055 Sankrit The Johns Hopkins University The Distribution of Shock Velocities in N49 - a Bright Supernova Remnant in the LMC C056 Bianchi The Johns Hopkins University Central Stars of Planetary Nebulae in the Small Magellanic Cloud C057 Murphy University of Virginia Observations of O VI Emission in the Halo of NGC 4631 C058 Hutchings NRC of Canada O stars in M33 C060 Froning Space Telescope Science Institute AM CVn Stars - Structure and Evolution of Ultra-Short Period Interacting Binaries C063 Bregman University of Michigan Is Gas Really Cooling in Cluster Cooling Flows C064 Bregman University of Michigan The Flow Velocities in Elliptical Galaxy Cooling Flows C067 Linsky University of Colorado Fluorescence and Excitation of Molecular Hydrogen in the Circumstellar Environment of PMS Stars C068 Long Space Telescope Science Institute Why do some Dwarf Novae Stand Still C070 OConnell University of Virginia The Disk-Halo Connection in the Spiral Galaxy M101 C072 Ghavamian Rutgers University A Far Ultraviolet Observation of the DEM L 71 Blast Wave C073 Boisse Ecole Normale SuperieureDEMIRM Probing the very small scale structure (l approx. 50 AU) in the interstellar medium (continued) C076 Howk The Johns Hopkins University Constraining the Scale of Variations in the Hot Interstellar Medium C078 Wood University of Colorado Observing the Accretion Disk Around Miras Companion in the FUV C079 Wood University of Colorado The O I and N I Abundance in the Local Interstellar Cloud C080 Kirshner Harvard University Far-Ultraviolet Spectra of a Supernova to be Named Later C081 Shull University of Colorado, Boulder Weighing the Low-Redshift Lyman alpha Forest C082 Lauroesch Northwestern University The Abundance of Interstellar Fluorine C083 Gaetz Harvard-Smithsonian Center for Astrophysic Probing the Reverse Shock in an Oxygen-Rich Supernova Remnant C084 Stocke University of Colorado, Boulder O VI Absorbers in Spiral Dominated Groups of Galaxies C086 Kraemer Catholic University of America FUSE Observations of the Dwarf Seyfert Nucleus of NGC 4395 C088 Lecavelier Institut dAstrophysique de Paris, CNRS A search for the 10^5--10^6 K gas in clusters of galaxies with massive cooling flow C090 Kriss Space Telescope Science Institute Simultaneous FUSE, HST, and Chandra Observations of Intrinsic Absorbers in NGC 7469 and Mrk 279 C092 Crenshaw Catholic University of America Simultaneous FUSE, HST, and Chandra Observations of the Seyfert Galaxies NGC 4151 and NGC 5548 C094 Szentgyorgyi CfA A FUSE Study of the Planetary Nebula NGC 246 C095 Ganguly The Pennsylvania State University Monitoring the Intrinsic Absorption Complex Toward RX J1230.8+0115 C096 Finley Eureka Scientific, Inc. The Influence of Weak Winds on DAO Abundances C097 Dufour Rice University The Wolf-Rayet Star HD 192163 And Its Surroundings C101 Guerrero University of Illinois O,VI Emission from the Cats Eye Nebula C102 Guinan Villanova University FUSE Observations of the Sun in Time - Transition Region Physics and Evolution of FUV Irradiances C103 Guinan Villanova University Eclipsing Binaries in the Large Magellanic Cloud Accurate Distances and Physical Properties C105 Bonamente University of Alabama in Huntsville FUSE observations of warm gas in clusters of galaxies and of Galactic OVI emission C106 Ayres University of Colorado Glimmers of Life in the Coronal Graveyard C107 Ayres University of Colorado Coronal Iron Survey The Yellow Giants C109 Bowen Princeton University A search for OVI absorption in the halo of the Large Magellanic Cloud C110 Sion Villanova University Probing White Dwarf Accretors and Inner Disk Structure of High Accretion Rate Dwarf Novae C111 Dupree Smithsonian Astrophysical Observatory An Evolving Trio of Hybrid Stars C113 Bianchi The Johns Hopkins University The Youngest, Massive Star Clusters in M33 C114 Brown University of Colorado Coronal Dynamics and Complete Flare Energy Budget for the M Dwarf AD Leo C116 Holberg University of Arizona A FUSE Determination of the Gravitational Redshift and Spectroscopic Mass of Sirius B C118 Fitzpatrick Villanova University The Atmospheres of High-Latitude Early B Stars C123 Reimers Universitat Hamburg Intergalactic Ionized Helium Absorption toward the UV-brightest high-z Quasar HS 1140+2711 C125 Henry The Johns Hopkins University Scattering From Interstellar Dust Near Stars C126 Grady Eureka Scientific Tracing the Molecular Environments of Herbig Ae Stars with FUSE C127 McCandliss The Johns Hopkins University Searching for Far-UV Fluorescence of Molecular Hydrogen in NGC 2023 C128 Brown GSFC How Does Abundance Affect the Strength of UV Emission in Elliptical Galaxies C129 Brown GSFC The Formation Mechanism of Helium-Rich Subdwarf B Stars C131 Hoopes Johns Hopkins University Probing the Coronal Gas in Starburst Superwinds Through O VI Emission C132 Bouret LAS de Marseille Probing Hot and Cold gas in Beta Pictoris Circumstellar Environment C134 De Marco American Museum of Natural History The Nova-Dwarf Nova Connection C138 Ake Johns Hopkins University Atmospheric Eclipsing Binaries HR6902 and 22Vul C140 King Space Telescope Science Institute FUSE Observations of Massive Evolved Stars in the LMC C141 Young Harvard-Smithsonian Center for Astrophysic RR Tel getting under the flux limit -- an observation with FUSE C149 Prochaska Carnegie Observatories Identifying the Physical Nature of Low z O,VI Absorbers C150 Shrader NASA Goddard Space Flight Center Far UV Spectroscopy of X-Ray Novae C151 St-Louis Universite de Montreal A Systematic Study of Colliding Winds in WR Stars. I. The Very-Short Period WC+O Binary HD36521 C152 Keyes Space Telescope Science Institute Outbursts in Symbiotic Binaries Z And Continued Observation C153 Shelton Johns Hopkins University Using FUSE to Measure the Galactic Halos O VI Intensity C154 Gull NASAs GSFC Eta Carinae Probing for the Physics C155 Owocki Univ. of Delaware The Physical Conditions in Grand Design Stellar Wind Variability C157 Peters University of Southern California A Study of the High Temperature Polar Plasma in B-Type Interacting Binaries C158 Peters University of Southern California Heavy Element Abundances in Two B0-B0.5 Main Sequence Stars in the Small Magellanic Cloud C160 Massa Goddard Space Flight Center The Metallicity Dependence of the Bistability Jump in Hot-Star Winds C161 Barrett Space Telescope Science Institute Time-resolved spectroscopy of high field polars C162 Barrett Space Telescope Science Institute Time-resolved spectroscopy of eclipsing polars C163 Shastri Indian Institute of Astrophysics Geometry of hot outflows in Seyfert galaxies C164 Korpela University of California, Berkeley Investigating OVI emission in the Eridanus Superbubble. C168 Bruhweiler The Catholic Univ. of America The NGC6164-5 & Rosette Nebulae Tests of the Theory for Interstellar Bubbles C169 Espey Space Telescope Science Institute FUSE Cycle 3 observations of the EG-AND eclipse ingress phases C171 Nichols Smithsonian Astrophysical Observatory Study of the Elongated Superbubble Around Cyg OB1 C172 Iping Catholic University of America The Hot ISM of the Antennae - The Nearest Galaxy Merger C176 Iping Catholic University of America Ionization Structure of the High-Excitation Planetary Nebula NGC 7009 C177 Werner Universitat Tubingen Temperature scale and metal abundances of hot hydrogen-rich central stars of planetary nebulae C178 Rauch Universitat Tubingen Exploring the evolutionary status of the O(He) stars