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Imaging Polarized Dust Emission in Star Formation Regions with the OVRO MM ArrayWe present OVRO interferometric observations of linearly polarized emission from magnetically aligned dust grains which allow the magnetic field geometry in nearby star formation regions to be probed on scales ranging from 100 to 3000 AU. Current results include observations of the young stellar objects NGC1333/IRAS 4A, IRAS 16293-2422 and Orion IRc2-KL.
Document ID
19970007831
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Akeson, Rachel
(California Inst. of Tech. Pasadena, CA United States)
Carlstrom, John
(California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 17, 2013
Publication Date
October 1, 1996
Publication Information
Publication: From Stardust to Planetesimals: Contributed Papers
Subject Category
Astronomy
Accession Number
97N14452
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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