Abstract
This paper presents observations of far infrared fine structure emission lines of OIII at 52 and 88 μm, 0I at 63 μm and NIII at 57 μm, obtained using a balloon borne telescope with a Michelson interferometer system. The sources M42 and M17 have been mapped with a beam of 1.6’ FWHM. Physical quantities derived from these measurements are presented and some of the results are discussed.
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© 1982 D. Reidel Publishing Company
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Naylor, D.A., Emery, R., Fitton, B., Furniss, I., Jennings, R.E., King, K.J. (1982). Fine Structure Lines in HII Regions Interacting with Molecular Clouds. In: Roger, R.S., Dewdney, P.E. (eds) Regions of Recent Star Formation. Astrophysics and Space Science Library, vol 93. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7778-5_10
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DOI: https://doi.org/10.1007/978-94-009-7778-5_10
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