Polarization of the Emission from M17: II. Comparison of Far-Infrared and Submillimeter Results

Details Polarization of the Emission from M17: II. Comparison of Far-Infrared and Submillimeter Results Polarization of the Emission from M17: II. Comparison of Far-Infrared and Submillimeter Results

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.1607d&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #16.07; Bulletin of the American Astronomical Society, Vol. 30, p.1277

Astronomy and Astrophysics

Astronomy

Scientific paper

We present polarization measurements at 60, 100, and 350 \micron\ of the M17 molecular cloud. A detailed comparison of the data sets is presented. On average, P(60)/P(100) = 1.2 and P(350)/P(100) = 0.4, but the actual dependence varies with location in the cloud. Scenarios to explain this behavior are discussed. We also examine the possibility that the magnetic field morphology has been driven by the expansion of the HII region into the molecular cloud.

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