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Molecular Line Observations in the Magellanic Clouds

Published online by Cambridge University Press:  25 May 2016

Lars E.B. Johansson ,
Arto Heikkilä  and
Hans Olofsson
Lars E.B. Johansson
Affiliation:
Onsala Space Observatory, S-439 92 Onsala, Sweden
Arto Heikkilä
Affiliation:
Onsala Space Observatory, S-439 92 Onsala, Sweden
Hans Olofsson
Affiliation:
Stockholm Observatory, S-133 36 Saltsjöbaden, Sweden

Abstract

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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 

References

Chin, Y.-N., Henkel, C., Millar, T.J., et al. 1998, A&A, 330, 901 Google Scholar
Heikkilä, A., Johansson, L.E.B., & Olofsson, H. 1999, A&A, 344, 817 Google Scholar
Johansson, L.E.B., Greve, A., Booth, R.S., et al. 1998, A&A, 331, 857 Google Scholar