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Submillimeter observations of the Orion Nebula and NGC 2024New observations at submillimeter wavelengths of the Orion Nebula and NGC 2024 are shown to provide a rather detailed map of the Orion Nebula at these wavelengths. The Orion Nebula emission is attributed to optically thin thermal radiation from dust grains in the molecular cloud with peak emission centered in the Kleinmann-Low nebula source.
Document ID
19740055734
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/181555
Authors
Soifer, B. T.
Hudson, H. S. (California, University San Diego, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
July 15, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 191
Subject Category
Space Sciences
Accession Number
74A38484
Funding Number(s)
CONTRACT_GRANT: NGL-05-009-230
CONTRACT_GRANT: NAS8-28015
Distribution Limits
Public
Copyright
Other

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