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A new, compact far-infrared source in the W31 regionIn a survey of the W31 region, a compact far-infrared source was detected at the position of the radio continuum source G 10.6-0.4. Associated with this infrared source and in close coincidence with its position is an H II region with a compact core and extended halo as well as OH and H2O masers. An extended molecular cloud, centered on these sources, has also been detected. The compact source and associated masers may be located at the H II region-molecular-cloud interface in a thin shocked layer of neutral gas driven into the molecular cloud by the expansion of the H II region. The compact H II region is depleted of dust and must be surrounded by a very dense shell of dust and gas (hydrogen number density in excess of 200,000 per cu cm). The source probably represents an early stage of stellar evolution.
Document ID
19780048589
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Fazio, G. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lada, C. J.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Kleinmann, D. E.
(Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Wright, E. L.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Ho, P. T. P.
(MIT Cambridge, Mass., United States)
Low, F. J.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
April 15, 1978
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
78A32498
Funding Number(s)
CONTRACT_GRANT: NSF AST-73-05042-A03
CONTRACT_GRANT: NGR-22-007-270
Distribution Limits
Public
Copyright
Other

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