High-resolution far-infrared observations of star-forming regions

Details High-resolution far-infrared observations of star-forming regions High-resolution far-infrared observations of star-forming regions

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phdt.........9c&link_type=abstract

Thesis (PhD). THE UNIVERSITY OF CHICAGO, Source DAI-B 60/02, p. 681, Aug 1999, 76 pages.

Computer Science

3

Scientific paper

We present new 60 and 100 μm observations of the massive star formation regions in the Orion Nebula (M42), M17, and NGC 6334, and of the bipolar nebula S106. Due to improvements in instrumentation and data reduction techniques, our images have the highest resolutions ever achieved at these wavelengths: 17'-18' at 60 μm and 27 '-29' at 100 μm. Compact objects are found in each region which were unresolved in previous studies; we estimate the luminosity and comment upon the nature of each of these sources.

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