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Chemical Abundances and Isotope Ratios in Molecular Clouds

Published online by Cambridge University Press:  25 April 2016

M. R. Hunt
M. R. Hunt*
Affiliation:
University of Western Sydney, Nepean, PO Box 10, Kingswood, NSW 2747, Australiamaria@st.nepean.uws.edu.au
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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.

Keywords

ISM: cloudsISM: moleculesgalaxies: interstellar mediumgalaxies: Magellanic Clouds
Type
Workshop on Millimetre-wave Astronomy
Information
Publications of the Astronomical Society of Australia , Volume 13 , Issue 2 , May 1996 , pp. 202 - 203
Copyright
Copyright © Astronomical Society of Australia 1996

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References

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