A good probe of molecular clouds and star-forming regions: CH 3CN
Abstract
Through our observations, analysis and calculations of the KL Region of Orion, we point out and illustrate the possibility and advantages of using the rotational lines of CH 3CN as a probe of molecular cloud cores and star-forming regions. We also discuss the instrumental requirements.
- Publication:
-
Chinese Astronomy and Astrophysics
- Pub Date:
- February 1996
- DOI:
- 10.1016/S0275-1062(96)00057-4
- Bibcode:
- 1996ChA&A..20..426Z