How does the Galaxy work?

Inhaltsverzeichnis

• The Milky Way: Four Centuries of Discovery of the Galaxy.
• Hi Clouds Beyond the Galactic Disk.
• The Wham Northern Sky Survey and the Nature of the Warm Ionized Medium in the Galaxy.
• The Structure of Galactic Hydrogen on the Largest Scales.
• The Bu-Fcrao Galactic Ring Survey.
• The View of the Interstellar Medium with the Canadian Galactic Plane Survey.
• Dark Hydrogen in the Galactic Plane.
• Diffuse Infrared Excess Features in the Canadian Galactic Plane Survey.
• The Oxygen Abundance in Our Galaxy.
• Ionization of the Galactic Halo.
• Diffuse Ionized Gas and the Disk-Halo Interaction in Spiral Galaxies.
• Are All the DIGs the Same?.
• Radio Halos in Star Forming Galaxies.
• Brackett-? Line Survey of the Ionized Hydrogen in the Galactic Plane.
• Leaky H II Regions and Heliumionization in the Reynolds Layer.
• Reynolds Layers in Nearby Galaxies: The Face-On View.
• Volume Filling Factors of the Dig.
• Latest Results of the Sethi Survey at Arecibo.
• Job Accomplished? The Escape of Ionizing Radiation from the Disks of Spiral Galaxies.
• Modeling the Diffuse Ionized Gas with Cloudy.
• Diffuse Ionized Medium Panel Discussion.
• Absorption Line Studies in the Halo.
• Dynamical Evolution of High Velocity Clouds in the Galactic Halo.
• Pulsar Bow Shocks as Probes of Warm Neutral Gas.
• Highly Ionized HVCs Towards Pks 2155–304: Galactic or Extragalactic?.
• Towards an Understanding of the Dynamics of the Milky Way.
• Fuse Observations of Ovi Emission from the Galactic Fountain.
• Pattern Speeds of Three Spirals Using Co and the Tremaine-Weinberg Method.
• Gas Infall Onto the Superthin Ic 2233.
• High-Velocity Gas Observed Towards the Shajn 147 Supernova Remnant.
• Hot Gas in the Galaxy.
• Bubbles and Superbubbles.
• The Chandra View of M101: What Can We Learn About the Milky Way?.
• Fuse Observationsof the Vela Supernova Remnant.
• Circumstellar Interaction in Young Radio Supernovae.
• Chandra Archive of Nearby Galaxies. I. Normal Galaxies.
• Hi Shells in the 2nd Galactic Quadrant.
• Key Science Programs for the Spear Mission.
• Chandra Archive of Nearby Galaxies. II. Galaxies with Nuclear Activity.
• Heating and Cooling in the ISM.
• The Galactic Centre and Its Black Hole.
• Stellar Metallicities and the Formation of the Galactic Bulge.
• The Galactic Bar.
• Stellar Distribution in the Galactic Disk from NIR Color-Magnitude Diagrams.
• Stellar Clusters in the Nucleus of Galaxie.
• Massive Young Clusters.
• Deep Multicolor NIR Surver of the Galactic Plane.
• Tracing the History of the Galaxy with Globular Clusters.
• Tidal Debris in the Galactic Halo.
• Star Formation in High-Redshift ISM.
• Gas Inflow in Spiral Galaxies from Kiloparsec to Parsec Scale.
• Open Clusters as Tracers of the Cygnus ARM.
• Triaxial Bulge and In-Plane Bar of the Milky Way.
• Tidal Shocks on Globular Clusters.
• Evolution of Globular Cluster Populations in Compact Galaxy Groups.
• Near IR Color-Magnitude Diagrams of Bulge Globular Clusters.
• Magnetic Fields in the Milky Way and Other Spiral Galaxies.
• The Origin of Galactic Magnetic Fields.
• Magnetic Turbulence in the WIM.
• Magnetic Fields and Spiral Structure.
• Calculations of the Dynamo Coefficients in Galactic Magnetic Fields with Shear.
• Galactic Magnetic Fields, from Radio Polarimetry of the WIM.
• Radio Polarimetry in the Sothern Galactic Plane Survey.
• The Truncation of the Stellar Disk of the Milky Way: A Magnetic Effect?.
• The Parker Instability.
• 3D MHD Modeling of the Galaxy.
• The Frequency Evolution of Interstellar Pulse Broadening from Radio Pulsars.
• 3D HD and MHD Adaptive Mesh Refinement Simulations of the Global and Local ISM.
• The Turbulent Interstellar Medium: Insights and Questions from Numerical Models.
• Hi: Temperatures, Magnetism, Turbulence, Morphology.
• Cosmic Rays and ? Rays in the Galaxy.
• Probing the Disk-Halo Connection Through the Local Interstellar Chimney.
• The Spear (Spectroscopy of Emission from Astrophysical Radiation) Mission.
• Dense Gas Contours Surrounding the Local Cavity: Comparison with the Soft X-Ray Background Emission Map.
• Fuse Observations of the Hot Post-AGB Star ZNG 1 in the Globular Cluster M5.
• 3D Simulations of the Local Bubble: How Much Ovi Can We Expect?.
• XMM-Newton Observations of the Local Bubble and the Galactic Halo.
• The Temperature of Massive Stars.
• Fuse Survey Of The Local Interstellar Medium.
• Diffuse Ovi Emission Towards the Loop I Superbubble.
• The Local Bubble: Where is the ?300,000 K Gas?.
• Is the Local Bubble Dead?.
• Closing Remarks.