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Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS resultsThe MILLIPOL polarimeter has been used to obtain 30-arcsec resolution 1300-micron data toward 10 cloud cores; the seven that were detected are associated with compact H II regions in massive molecular clouds. Cloud-core axis ratios and position angles were derived by examining the morphologies of IRAS-traced dust opacity structures. The MILLIPOL-detected cloud cores exhibit 1.5-3.2 core axis ratio values. The magnetic field is found to be generally perpendicular to the core dust distributions.
Document ID
19930062231
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kane, Brian D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Clemens, Dan P.
(Boston Univ. MA, United States)
Barvainis, Richard
(Haystack Observatory Westford, MA, United States)
Leach, Robert W.
(San Diego State Univ. CA, United States)
Date Acquired
August 16, 2013
Publication Date
July 10, 1993
Publication Information
Publication: Astrophysical Journal - Part 1
Volume: 411
Issue: 2
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A46228
Funding Number(s)
CONTRACT_GRANT: NAG5-1160
Distribution Limits
Public
Copyright
Other

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