The magnetic field is a key ingredient in the recipe of star formation. However, the
importance of the magnetic field in the early stages of the formation of low-and high-mass …

Star formation is a multi-scale, multi-physics problem ranging from the size scale of
molecular clouds (∼ 10 ∼10 s pc) down to the size scales of dense prestellar cores (∼ 0.1 …

In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …

Abstract We present 0 farcs 25 resolution (35 au) ALMA 1.3 mm dust polarization
observations for 37 young stellar objects (YSOs) in the Ophiuchus molecular cloud. These …

Abstract The Davis–Chandrasekhar–Fermi (DCF) method provides an indirect way to
estimate the magnetic field strength from statistics of magnetic field orientations. We compile …

We present new observations of the active star formation region NGC 1333 in the Perseus
molecular cloud complex from the James Clerk Maxwell Telescope B-Fields In Star-forming …

Observations of star-forming regions by the current and upcoming generation of
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …

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 850 μm polarization observations of the L1689 molecular cloud, part of the
nearby Ophiuchus molecular cloud complex, taken with the POL-2 polarimeter on the James …