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The Orion Molecular Cloud at Far-infrared WavelengthsA new, 34 in resolution far-infrared continuum map of Orion Molecular Cloud 1 and its environs, including M43 is presented. The source is dominated by a single, bright peak at the position of the embedded infrared cluster, with the 60 micro m flux density falling off steeply in all directions away from it. A total luminosity for IRc2 of 20,000 L(solar) is estimated, although this may be a lower limit, depending upon the transfer of radiation in the vicinity of the object. Several condensations appear in this map, which, along with radio molecular observations, support the view that significant fragmentation has taken place within the cloud.
Document ID
19850009551
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Thronson, H. A., Jr.
(Wyoming Univ. Laramie, WY, United States)
Harper, D. A.
(Chicago Univ. Berkeley, United States)
Smith, H. A.
(Naval Research Lab. Laramie, WY, United States)
Schwartz, P. R.
(Naval Research Lab.)
Lada, C. J.
(Arizona Univ.)
Bally, J.
(Bell Labs.)
Bieging, J. H.
(California Univ.)
Greenhouse, M.
(Wyoming Univ.)
Loewenstein, R. F.
(Chicago Univ.)
Date Acquired
August 12, 2013
Publication Date
December 1, 1984
Publication Information
Publication: NASA. Ames Research Center Airborne Astron. Symp.
Subject Category
Astronomy
Accession Number
85N17860
Funding Number(s)
CONTRACT_GRANT: NAG2-134
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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