AASTCS 4: Workshop on Dense Cores: Origin, Evolution, and Collapse
Overview
AASTCS
4
Workshop on Dense Cores: Origin, Evolution, and Collapse
Monterey, CA
27
–
30 July 2014
The AASTCS 4 Meeting was held 27 - 30 July 2014 at the Hyatt Regency, Monterey, CA.
View Presentations from AASTCS 4
- 100.01 Philippe Andre: Herschel Observations of Gould Belt Cores and Filaments
- 106.01 Enrique Vazquez-Semadeni: Formation and Evolution of Cores in Globally Collapsing Environments
- 107.01 Scott Schnee: A Search For Fragmentation in Starless Cores with ALMA
- 107.02 Shaye Storm: Large Area, High Resolution N2H+ Studies of Dense Gas in the Perseus and Serpens Molecular Clouds
- 201.01 James Di Francesco: Identification of Super-Jeans Mass Cores
- 202.01Chang Won Lee: Inward Motions in Dense Molecular Cores
- 204.01 Jaime Pineda: The First ALMA View of IRAS 16293-2422: Infall and Rotation
- 206.02 Ramprasad Rao: Detection of a Magnetized Disk Around a Very Young Protostar
- 207.01 Søren Frimann: Bridging the Gap between Large-Scale Simulations and Observations of Star Forming Cores
- 207.02 Sarah Sadavoy: Evidence of Feedback? A Correlation Between Class 0 Protostars and the Dense Gas Distribution in the Perseus Molecular Cloud
- 207.03 Raghvendra Sahai: Shocked and Scorched - Free-Floating Evaporating Gas Globules and StarFormation
- 207.04 Yao-Lun Yang: Study of Outflow and Molecular Lines from the Observations of BHR71 by The Herschel Key Program,``Dust, Ice, and Gas In Time" (DIGIT)
- 207.05 Christopher Tibbs: Using Spinning Dust Emission to Constrain The Abundance Of Small Dust Grains In Dense Cores
- 300.01 Rowan Smith: Modeling Massive Star Formation
- 302.01 Qizhou Zhang: Fragmentation of Molecular Clumps and Formation of Massive Cores
- 305.01 John Bally: Clumps & Cores in Massive Star-Forming Regions from Orion to the Central Molecular Zone
- 307.02 Peter Barnes: Physical Conditions and Star Formation in Cluster-Forming Molecular Clumps
- 307.05 Randolf Klein: Issues with SED fitting, PMS Tracks, and the Birthline Exemplified with Two Cores Near IRAS 05345+3157