Showing 1–20 of 21 results
/ Date/ Name
Mar 26, 2018OH as an Alternate Tracer for Molecular Gas: Excitation Temperatures of the OH 18-cm Main Lines in W5Feb 2, 2015The Structure of Dark Molecular Gas in the Galaxy - I: A Pilot Survey for 18-cm OH Emission Towards $l \approx 105^°, b \approx +1^°$Feb 20, 2012Faint Extended OH Emission from the Local Interstellar Medium in the Direction l \approx 108\circ, b \approx 5\circJan 13, 2012Radio & Optical Interferometry: Basic Observing Techniques and Data AnalysisMar 13, 2009Mass Transport Processes and their Roles in the Formation, Structure, and Evolution of Stars and Stellar SystemsAug 4, 2008The volume densities of giant molecular clouds in M83May 29, 2008Crowded-Field Astrometry with SIM PlanetQuest. II. An Improved Instrument ModelJul 2, 2007Station-Keeping Requirements for Constellations of Free-Flying Collectors Used for Astronomical Imaging in SpaceApr 2, 2007A Comparison between Anomalous 6-cm H$_2$CO Absorption and CO(1-0) Emission in the L1204/S140Jul 27, 2006Anomalous H_2CO Absorption Towards the Galactic Anticenter: A Blind Search for Dense Molecular CloudsNov 24, 2004The Opacity of Spiral Galaxy Disks IV: Radial Extinction Profiles from Counts of Distant Galaxies seen through Foreground DisksNov 24, 2004The Opacity of Spiral Galaxy Disks III: Automating the "Synthetic Field Method"Jun 30, 2004Photodissociation and the Morphology of HI in GalaxiesMar 16, 2004Cold Molecular Gas as a Possible Component of Dark Matter in the Outer Parts of Disk GalaxiesFeb 16, 2004The Production of HI in Photodissociation Regions and A Comparison with CO(1-0) EmissionMay 13, 2002On The Origin of HI in Galaxies: Photodissociation and the ``Schmidt Law'' for Global Star FormationMar 6, 2002On The Origin Of HI In Galaxies: The Sizes and Masses of HI Photodissociation RegionsJun 22, 2001The Formation of Molecular CloudsMar 1, 2001Cold Molecular Gas, PDRs, and the Origin of HI in GalaxiesFeb 21, 2001Gas, Dust, and Young Stars in the Outer Disk of M 31