Molecular Line Observations in the Large Magellanic Cloud

Details Molecular Line Observations in the Large Magellanic Cloud Molecular Line Observations in the Large Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..397g&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

7

Scientific paper

A summary report on current observing programs of the LMC at various
CSIRO facilities is presented. Molecular-line observations include OH at
18 cm, H2CO at 6 cm, CH at 9 cm, H2O at 1.3 cm,
HCO+ at 3.4 mm and CO at 2.6 mm.

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