4 papers
Molecules in Southern Dense Cores I: Mopra and SEST Millimetre-Wave Observations
Maria R. Hunt Cunningham, John B. Whiteoak, Paul A. Jones +1
We have observed molecular-line transitions between 84 and 147 GHz in 24 dense southern molecular clouds with declinations south of -30 degrees using the Mopra and SEST radio teles…
Molecular abundances in the Magellanic Clouds III. LIRS 36, a star-forming region in the SMC
Y. -N. Chin, C. Henkel, T. J. Millar +2
Detections of CO, CS, SO, C2H, HCO+, HCN, HNC, H2CO, and C3H2 reported from LIRS 36, a star-forming region in the Small Magellanic Cloud. C18O, NO, CH3OH, and most notably CN have…
Molecular abundances in the Magellanic Clouds II. Deuterated species in the LMC
Y. -N. Chin, C. Henkel, T. J. Millar +2
The first definite discoveries of extragalactic deuterium are reported. DCO has been detected in three and DCN has been measured in one star-forming region of the Large Magella…
Molecular abundances in the Magellanic Clouds I. A multiline study of five cloud cores
Y. -N. Chin, C. Henkel, J. B. Whiteoak +3
Nine HII regions of the LMC were mapped in 13CO(1--0) and three in 12CO(1--0) to study the physical properties of the interstellar medium in the Magellanic Clouds. For N113 the mol…