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 …

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 expand our study on the dispersion of polarization angles in molecular clouds. We show
how the effect of signal integration through the thickness of the cloud as well as across the …

We investigate the interplay between magnetic (B) field, gravity, and turbulence in the
fragmentation process of cores within the filamentary infrared dark cloud G34. 43+ 00.24 …

We report the detection of variable emission from Sgr A* in almost all wavelength bands (ie,
centimeter, millimeter, submillimeter, near-IR, and X-rays) during a multi-wavelength …

Modern understanding of dust astrophysics reveals that radiative torques (RATs) arising
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …

With the forthcoming release of high precision polarization measurements, such as from the
Planck satellite, it becomes critical to evaluate the performance of estimators for the …

We present 350 μm polarization observations of four low-mass cores containing Class 0
protostars: L483, L1157, L1448-IRS2, and Serp-FIR1. This is the second paper in a larger …

As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop
a greater understanding for the complex relationships between the large-scale diffuse gas …

We present the first detection of polarization around the Class 0 low-mass protostar L1157-
mm at two different wavelengths. We show polarimetric maps at large scales (10''resolution …