The submillimeter polarization spectrum of M17

Lingzhen Zeng, Charles L. Bennett, Nicholas L. Chapman, David T. Chuss, Izaskun Jimenez-Serra, Giles Novak, John E. Vaillancourt

Research output: Contribution to journalArticle

9 Scopus citations

Abstract

We present 450 μm polarimetric observations of the M17 molecular cloud obtained with the SHARP polarimeter at the Caltech Submillimeter Observatory. Across the observed region, the magnetic field orientation is consistent with previous submillimeter and far-infrared polarization measurements. Our observations are centered on a region of the molecular cloud that has been compressed by stellar winds from a cluster of OB stars. We have compared these new data with previous 350 μm polarimetry and find an anti-correlation between the 450 and 350 μm polarization magnitude ratio and the ratio of 21 cm to 450 μm intensity. The polarization ratio is lower near the east end of the studied region where the cloud is exposed to stellar winds and radiation. At the west end of the region, the polarization ratio is higher. We interpret the varying polarization spectrum as evidence supporting the radiative alignment torque model for grain alignment, implying higher alignment efficiency in the region that is exposed to a higher anisotropic radiation field.

Original languageEnglish (US)
Article number29
JournalAstrophysical Journal
Volume773
Issue number1
DOIs
StatePublished - Aug 10 2013

Keywords

  • ISM: clouds
  • ISM: individual objects (M17, NGC 6618)
  • ISM: magnetic fields
  • polarization
  • submillimeter: ISM

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Zeng, L., Bennett, C. L., Chapman, N. L., Chuss, D. T., Jimenez-Serra, I., Novak, G., & Vaillancourt, J. E. (2013). The submillimeter polarization spectrum of M17. Astrophysical Journal, 773(1), [29]. https://doi.org/10.1088/0004-637X/773/1/29