136912-Thumbnail Image.png
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

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.
1.06 MB application/pdf

Download restricted. Please sign in.
Restrictions Statement

Barrett Honors College theses and creative projects are restricted to ASU community members.

Details

Title
  • Searching for Stellar Outflow in the R Coronae Australis Region
Contributors
Date Created
2014-05
Resource Type
  • Text
  • Machine-readable links