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M17 SW molecular cloud

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/161028· OSTI ID:5471235
We report new /sup 12/CO and /sup 13/CO observations of the massive molecular cloud associated with the giant M17 H II region. With a spatial resolution higher than previously reported, we find the brightest /sup 12/CO emission to lie in an elongated ridge, parallel and adjacent to a sharp ionization front at the apparent H II/H/sub 2/ interface. To within the positional uncertainties, the highest temperature /sup 12/CO emission is coincident with the brightest 100 ..mu..m emission. That this was not seen in earlier, lower resolution /sup 12/CO maps suggests a very steep molecular temperature gradient across the ionization front and emphasizes the uncertainties of using finite-sized beams. With the new data the molecular dissociation front is located. The radio molecular data also support the idea of a dusty molecular cloud that is largely externally heated by the exciting stars of the M17 H II region. These enormously luminous stars may be masking significant star-forming activity within the molecular cloud itself. The conditions in this cloud are suitable for star formation, although investigating this process in the infrared may be extremely difficult: /sup 13/CO column densities indicate significant absorption optical depths at wavelengths as long as approx.50 ..mu..m.
Research Organization:
Wyoming Infrared Observatory, University of Wyoming
OSTI ID:
5471235
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 269:1; ISSN ASJOA
Country of Publication:
United States
Language:
English

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