Molecular line mapping of OMC-1
Abstract
New, fully sampled maps of the molecular emission from CO, (C-13)O, and HCN in the Orion Molecular Cloud are presented. The high resolution of the maps (less than 1 arcmin) reveals considerable structure in the molecular gas that is related to the H II region surrounding the Trapezium.
- Publication:
-
Regions of Recent Star Formation
- Pub Date:
- 1982
- DOI:
- 10.1007/978-94-009-7778-5_58
- Bibcode:
- 1982ASSL...93..439S
- Keywords:
-
- Astronomical Maps;
- Molecular Clouds;
- Molecular Spectra;
- Orion Nebula;
- Brightness Temperature;
- Carbon Monoxide;
- Emission Spectra;
- H Ii Regions;
- Hydrocyanic Acid;
- Astrophysics