Models and Observations of the Millimeter and Submillimeter Molecular Line Emission of Bright-Rimmed Clouds
Current Topics: Lyman Break Galaxies - Lecture 2 Current Topics Lyman Break Galaxies Dr Elizabeth Stanway ([email protected])
Propagation of highly_efficient_star_formation_in_ngc7000
Background We selected the CG4 environment within the Gum Nebula because the area is visually dense with star- forming material. CG4 ( 07 h 32 m 45 s,
CO, CS or other molecules? Maria Cunningham, UNSW.
How Unique Are Nearby Debris Disks? Alycia Weinberger (DTM/CIW)
VLASS – Galactic Science Life cycle of star formation in our Galaxy as a proxy for understanding the Local Universe legacy science Infrared GLIMPSE survey.
Westerlund 1 Ignacio Negueruela Santiago 2006 Starburst in our backyard.
Background .
OB Spectral and Spatial Morphology from Carina to the Antennae
Massive Star Formation under Different Z & Galactic Environment
ICM-ISM Stripping in Virgo Cluster Spiral Galaxies Jeff Kenney (Yale University) with: J. Van Gorkom B. Vollmer H. Crowl * A. Abramson A. Chung J. Cortes.
