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ISO Observations of Compact HII Regions in the Large Magellanic Cloud1

Published online by Cambridge University Press:  25 May 2016

A. Moneti ,
R. J. Laureijs ,
J.M. van der Hulst ,
F. Israel  and
P.P. van der Werf
A. Moneti
Affiliation:
ISO Data Centre, VILSPA, 28080 Spain
R. J. Laureijs
Affiliation:
ISO Data Centre, VILSPA, 28080 Spain
J.M. van der Hulst
Affiliation:
Kapteyn Astronomical Institute, 9700-AV Groningen, The Netherlands
F. Israel
Affiliation:
Sterrewacht, 2300-RA Leiden, The Netherlands
P.P. van der Werf
Affiliation:
Sterrewacht, 2300-RA Leiden, The Netherlands

Abstract

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With the detection of strong PAH features and H2 emission in selected knots of the N159, N11A, and 30 Dor regions in the LMC, we present the first results of a study that is part of a coordinated Guaranteed Time ISO programme to investigate star formation in the Magellanic Clouds. The PAH features have different ratios than the ones in Galactic reflection nebulae.

Type
Part 5. Stellar Populations and Surveys
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 377 - 378
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Israel, F.P., & Koornneef, J. 1991, A&A, 250, 475 Google Scholar
Johansson, L.E.B., et al. 1998, A&A, 331, 857 Google Scholar