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The far-infrared polarization of the Orion nebulaPolarization of the 100 micron thermal emission from 10 points in the Orion nebula has been measured. At one of the positions the degree, 5.7 percent, is the largest far-infrared polarization yet discovered. Except at a position in the barlike structure to the south, the position angles of the polarization vectors are well-ordered, suggesting that a uniform magnetic field threads the cloud. The magnetic field strength is estimated to be between 0.7 and 4 mG. The relationship of the degrees of polarization to the physical conditions in the cloud is discussed.
Document ID
19900052185
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Gonatas, D. P.
(Chicago Univ. Chicago, IL, United States)
Engargiola, G. A.
(Chicago Univ. Chicago, IL, United States)
Hildebrand, R. H.
(Chicago Univ. Chicago, IL, United States)
Platt, S. R.
(Chicago Univ. Chicago, IL, United States)
Wu, X. D.
(Chicago, University IL, United States)
Davidson, J. A.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 14, 2013
Publication Date
July 1, 1990
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 357
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
90A39240
Funding Number(s)
CONTRACT_GRANT: NSG-2057
Distribution Limits
Public
Copyright
Other

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