Searching for Stellar Outflow in the R Coronae Australis Region
Description
Using data from the Arizona Radio Observatory Submillimeter Telescope, we have studied the active, star-forming region of the R Coronae Australis molecular cloud in 12CO (2-1), 13CO (2-1), and HCO+ (3-2). We baselined and mapped the data using CLASS. It was then used to create integrated intensity, outflow, and centroid velocity maps in IDL. These clearly showed the main large outflow, and then we identified a few other possible outflows.
Date Created
The date the item was original created (prior to any relationship with the ASU Digital Repositories.)
2014-05
Agent
- Author (aut): Blumm, Margaret Elizabeth
- Thesis director: Groppi, Christopher
- Committee member: Bowman, Judd
- Committee member: Mauskopf, Philip
- Contributor (ctb): Barrett, The Honors College
- Contributor (ctb): School of Earth and Space Exploration