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• W1990197659 abstract "We present spectropolarimetry, and 12- and 2-μm imaging polarimetry of the southern massive star-forming region G333.6−0.2. Spectro-polarimetry measurements show that the polarization observed towards the nebula contains a mixture of both absorptive and emissive polarizations. Model fitting to the spectra indicates that the temperature of the mid-infrared emitting dust grains is generally ∼200 K and the optical depth of the absorbing dust at 9.7 μm is ∼1.5. Fits are also made to the polarimetry spectra, which show a reasonably constant peak absorptive polarization (∼3.4 per cent at 43°) across the face of the H ii region. This absorptive polarization position angle is consistent with that found by the 2-μm imaging polarimetry and is most likely due to the Galactic magnetic field local to G333.6−0.2. When the absorptive polarization is subtracted from the 12-μm polarization image, the emissive polarization pattern that is intrinsic to the star-forming region is revealed. A probable magnetic field configuration implied by the intrinsic polarization suggests star formation initially influenced by the Galactic magnetic field which is eventually perturbed by the star formation process." @default.
• W1990197659 created "2016-06-24" @default.
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• W1990197659 date "2001-10-01" @default.
• W1990197659 modified "2023-10-06" @default.
• W1990197659 title "Infrared polarimetry of the southern massive star-forming region G333.6−0.2" @default.
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• W1990197659 doi "https://doi.org/10.1046/j.1365-8711.2001.04704.x" @default.
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