Interstellar polarization at optical-to-infrared wavelengths is known to arise from asymmetric
dust grains aligned with the magnetic field. This effect provides a potentially powerful probe …

Here we present deep (16 μJy beam− 1), very high (40 mas) angular resolution 1.14 mm,
polarimetric, Atacama Large Millimeter/submillimeter Array (ALMA) observations toward the …

Polarization arising from aligned dust grains presents a unique opportunity to study
magnetic fields in the diffuse interstellar medium and molecular clouds. Polarization from …

We report on the highest spatial resolution measurement to date of magnetic fields (B-fields)
in M17 using thermal dust polarization measurements taken by SOFIA/HAWC+ centered at a …

We present the results of simultaneous 450 μm and 850 μm polarization observations
toward the massive star-forming region NGC 2071IR, a target of the BISTRO (B-fields in …

Polarized emission from aligned dust is a crucial tool for studies of magnetism in the ISM, but
a troublesome contaminant for studies of cosmic microwave background polarization. In …

Polarization maps of the Vela C molecular cloud were obtained at 250, 350, and 500 μm
during the 2012 flight of the balloon-borne telescope BLASTPol. These measurements are …

We report on polarimetric maps made with HAWC+/SOFIA toward ρ Oph A, the densest
portion of the ρ Ophiuchi molecular complex. We employed HAWC+ bands C (89 μm) and D …

Linear polarization maps of the Carina Nebula were obtained at 250, 350, and 500 μm
during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for …

We analyze the wavelength dependence of the far-infrared polarization fraction toward the
OMC-1 star-forming region using observations from HAWC+/SOFIA at 53, 89, 154, and 214 …