Atomic hydrogen (Hi) is a critical step** stone in the gas evolution cycle of the interstellar
medium (ISM) of the Milky Way. Hi traces both the cold, premolecular state before star …

Cosmic inflation provides a window to the highest energy densities accessible in nature, far
beyond those achievable in any realistic terrestrial experiment. Theoretical insights into the …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

Recent measurements of Galactic polarized dust emission have found a nonzero TB signal,
a correlation between the total intensity and the B-mode polarization component. We …

If a single line of sight (LOS) intercepts multiple dust clouds with different spectral energy
distributions and magnetic field orientations, then the frequency scaling of each of the …

We report on the design and performance of the B icep3 instrument and its first three-year
data set collected from 2016 to 2018. B icep3 is a 52 cm aperture refracting telescope …

The change of physical conditions across the turbulent and magnetized interstellar medium
induces a 3D spatial variation of the properties of Galactic polarized emission. The observed …

The alignment of striated intensity structures in thin neutral hydrogen (H i) spectroscopic
channels with Galactic magnetic fields has been observed. However, the origin and nature …

To investigate the role of magnetic fields in the evolution of the interstellar medium,
formation and evolution of molecular clouds, and ultimately the formation of stars, their three …

The complex interplay of magnetohydrodynamics, gravity, and supersonic turbulence in the
interstellar medium (ISM) introduces a non-Gaussian structure that can complicate a …