Chemical abundances and isotope ratios in molecular clouds

Details Chemical abundances and isotope ratios in molecular clouds Chemical abundances and isotope ratios in molecular clouds

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pasa...13..202h&link_type=abstract

Publications Astronomical Society of Australia, vol. 13, no. 2, p. 202-203

Astronomy and Astrophysics

Astronomy

Ism, Galaxies, Magellanic Clouds

Scientific paper

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.

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