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The magnetic field structure in high-mass star formation regionsWe present a preliminary analysis of far-IR polarimetric observations, which were made to study the magnetic field structure in the high-mass star formation regions of M42, NGC2024, and W3. These observations were made from the Kuiper Airborne Observatory (KAO), using the University of Chicago far-IR polarimeter, Stokes.
Document ID
19960003643
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Davidson, Jacqueline A.
(Search for Extraterrestrial Intelligence Inst. Mountain View, CA, United States)
Schleuning, D.
(Chicago Univ. Chicago, IL., United States)
Dotson, J. L.
(Chicago Univ. Chicago, IL., United States)
Dowell, C. Darren
(Chicago Univ. Chicago, IL., United States)
Hildebrand, Roger H.
(Chicago Univ. Chicago, IL., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Astronomical Society of the Pacific, Airborne Astronomy Symposium on the Galactic Ecosystem: From Gas to Stars to Dust, Volume 73
Subject Category
Astrophysics
Accession Number
96N13653
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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