The formation of protostars and their disks has been understood as the result of the
gravitational collapse phase of an accumulation of dense gas that determines the mass …

Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …

GRB 221009A was the brightest gamma-ray burst ever detected on Earth. In its early
afterglow phase, photons with exceptional energies above 10 TeV were observed by …

Stars form from the gravitational collapse of turbulent, magnetized molecular cloud cores.
Our non-ideal MHD simulations reveal that the intrinsically anisotropic magnetic resistance …

We present 500 and 700 au resolution 1 and 3 mm Atacama Large Millimeter/submillimeter
Array observations, respectively, of protostellar cores in protoclusters Sagittarius B2 (Sgr B2) …

Abstract We report on Atacama Large Millimeter/submillimeter Array observations of
polarized dust emission at 1.2 mm from NGC6334I, a source known for its significant flux …

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 …

Context. Magnetic fields are predicted to have a crucial impact on the structure, evolution,
and chemistry of protoplanetary disks. However, a direct detection of the magnetic field …

ABSTRACT Cold (10 K) and dense (cm) cores of gas and dust within molecular clouds,
known as starless and dynamically evolved pre-stellar cores, are the birthplaces of low …

Context. Turbulence is a key component of molecular cloud structure. It is usually described
by a cascade of energy down to the dissipation scale. The power spectrum for subsonic …