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Observations of the 89 GHz Transition of HCO+ in Orion
Published online by Cambridge University Press: 25 April 2016
Extract
Observations of CO emission (Kutner et al. 1977) have delineated a molecular cloud extending over several square degrees in the Orion region, and extensive surveys have been made of several other molecules (e.g. CN, CS, HCN, H2CO, H2H+) in the densest regions of this cloud.
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- Copyright © Astronomical Society of Australia 1980
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