Abstract
Observational and theoretical results over the last few years have highlighted the interrelationship between OB stars, ultracompact H II regions and molecular clouds. We review recent observational data and models for ultracompact H II regions, and show where the data fit and do not fit the models which have been designed to explain them.
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© 1990 Springer-Verlag
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Gaume, R.A. (1990). The relation between OB stars, H II regions & molecular clouds. In: Wilson, T.L., Johnston, K.J. (eds) The Structure and Content of Molecular Clouds 25 Years of Molecular Radioastronomy. Lecture Notes in Physics, vol 439. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3540586210_14
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DOI: https://doi.org/10.1007/3540586210_14
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