We present 850 μm dust polarization observations of the massive DR21 filament from the B-
fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter …

We present 850 μm polarimetric observations toward the Serpens Main molecular cloud
obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope as part of the …

We present observations of polarized dust emission at 850 μm from the L43 molecular
cloud, which sits in the Ophiuchus cloud complex. The data were taken using SCUBA-2/POL …

We present and analyze observations of polarized dust emission at 850 μm toward the
central 1× 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obtained …

Simulations of molecular clouds often begin from highly idealized initial conditions, such as
a uniform-density sphere with an artificially imposed turbulent velocity field. While the …

Direct observational measurements of the magnetic field strength in pre-stellar cores
typically find supercritical mass-to-flux ratios, suggesting that the magnetic field is insufficient …

We present the results of 850 μm polarization and C 18 O (3− 2) line observations toward
the western hub-filament structure (W-HFS) of the dark Streamer in IC 5146 using the James …

We have observed the large Bok globule CB 54 in 850-m polarized light using the POL-2
polarimeter on the James Clerk Maxwell Telescope (JCMT). We find that the magnetic field …

Polarized dust emission is a key tracer in the study of interstellar medium and of star
formation. The observed polarization, however, is a product of magnetic field structure, dust …

We present BISTRO Survey 850 μm dust emission polarization observations of the L1495A-
B10 region of the Taurus molecular cloud, taken at the James Clerk Maxwell Telescope …