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Molecular Line Observations in the Magellanic Clouds
Published online by Cambridge University Press: 25 May 2016
Abstract
We have observed spectral line emission from a sample of clouds in the Magellanic Clouds to investigate the effects of metallicity and FUV radiation on the physical and chemical properties of the interstellar medium. The clouds were identified by CO surveys and selected to cover a wide range of environments. We present molecular line data for five clouds in the LMC and one cloud in the SMC.
- Type
- Part 2. Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 116 - 117
- Copyright
- Copyright © Astronomical Society of the Pacific 1999