Imaging polarized dust emission in star formation regions with the OVRO mm array.

Details Imaging polarized dust emission in star formation regions with the OVRO mm array. Imaging polarized dust emission in star formation regions with the OVRO mm array.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339...45a&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 45 - 48

Physics

Star-Forming Regions: Polarization, Star-Forming Regions: Dust Grains

Scientific paper

The authors 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 NGC 1333/IRAS 4A, IRAS 16293-2422 and Orion IRc2-KL.

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