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 …

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 …

Context. Electron fraction and cosmic-ray ionization rates in star-forming regions are
important quantities in astrochemical modeling and are critical to the degree of coupling …

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

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 …

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 …

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 …

Magnetic fields are ubiquitous in the Universe and are thought to play an important role in
various astrophysical processes. Polarization of thermal emission from dust grains aligned …

We have comprehensively studied the multiscale physical properties of the massive infrared
dark cloud G28. 34 (the Dragon cloud) with dust polarization and molecular line data from …

Understanding the physical processes that regulate star formation and galaxy evolution are
major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to …