How does the Galaxy Work? A Galactic Tertulia with Don Cox and Ron Reynolds /
| Συγγραφή απο Οργανισμό/Αρχή: | |
|---|---|
| Άλλοι συγγραφείς: | , , |
| Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
| Γλώσσα: | English |
| Έκδοση: |
Dordrecht :
Springer Netherlands,
2005.
|
| Σειρά: | Astrophysics and Space Science Library ;
315 |
| Θέματα: | |
| Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- 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 Observations of 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.
