Posters
Poster 1: | The BU-FCRAO Galactic Ring Survey: The Channel Maps | |
Poster 2: | Infrared Dark
Clouds in the BU-FCRAO Milky Way Galactic Ring Survey |
|
Poster 3 : | HI Self Absorption
Toward Molecular Clouds: Theoretical Models |
|
Poster 4 : | The Structure of GRSMC 045.46+0.05 |
Poster 1: | The Radial Distribution of Cold HI in the Galaxy | |
Poster 2: | Infrared Dark
Clouds in the BU-FCRAO Milky Way Galactic Ring Survey |
Poster 1: |
Breaking the Near-Far
Kinematic Distance Ambiguity
|
|
Poster 2: |
Principal
Component and Delta-Variance Analysis of large scale spectral line
images of clouds in the first Galactic quadrant
|
|
Poster 3: |
Finding
Near Molecular Clouds in the Galaxy
|
Poster 1: | Structure and Equilibrium of Four Molecular Clouds in the GRS | |
Poster 2: | Resolving the Near-Far Kinematic Distance Ambiguity | |
Poster 3: | Determining the Distances to Infrared Point Sources | |
Poster 4: | Comparison of CS with 13CO Emission |
Poster 1: | The first two Square Degrees | |
Poster 2: | Kinematics and Correlation with the Optical, H I, and Infrared |
The GRS is supported by the NSF via grant AST-9800334 and AST-0098562 |