The Galactic Magnetic Field's Effect In Star-Forming Regions
Abstract
We investigate the effect of the Milky Way's magnetic field in star-forming regions using archived 350μm polarization data on 52 Galactic star formation regions from the Hertz polarimeter module. The polarization angles and percentages for individual telescope beams were combined in order to produce a large-scale average for each source and for complexes of sources. In more than 80% of the sources, we find a meaningful mean magnetic field direction, implying the existence of an ordered magnetic field component at the scale of these sources. The average polarization angles were analyzed with respect to the Galactic coordinates in order to test for correlations between polarization percentage, polarization angle, intensity, and Galactic location. No correlation was found, which suggests that the magnetic field in dense molecular clouds is decoupled from the large-scale Galactic magnetic field. Finally, we show that the magnetic field directions in the complexes are consistent with a random distribution on the sky.
Additional Information
© 2011 American Astronomical Society. Received 2010 September 6; accepted 2010 December 13; published 2011 January 25. Part of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. L.W.L. acknowledges support from the National Science Foundation under grant no. AST-07- 09206. We also acknowledge Richard M. Crutcher for extensive discussions.Attached Files
Published - Stephens2011p13137Astrophys_J.pdf
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Additional details
- Eprint ID
- 23009
- Resolver ID
- CaltechAUTHORS:20110321-102826137
- NASA
- AST-07-09206
- NSF
- Created
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2011-03-21Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field