Chemical abundances and isotope ratios in molecular clouds
Abstract
A program to observe millimetre-wave molecular transitions in a number of southern-sky molecular clouds is under way. Molecular clouds in both The Galaxy and The Magellanic Clouds are included in the sample. The aim of the program is to build a body of observational data which can be used to derive molecular abundances in southern sky molecular clouds.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- May 1996
- DOI:
- 10.1017/S132335800002083X
- Bibcode:
- 1996PASA...13..202H
- Keywords:
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- ISM;
- GALAXIES;
- MAGELLANIC CLOUDS