For decades we have known that the Sun lies within the Local Bubble, a cavity of low-
density, high-temperature plasma surrounded by a shell of cold, neutral gas and dust …

Leveraging a high-resolution 3D dust map of the solar neighborhood from Edenhofer et al.,
we derive a new 3D model for the dust-traced surface of the Local Bubble, the supernova …

Abstract PHANGS–JWST mid-infrared (MIR) imaging of nearby spiral galaxies has revealed
ubiquitous filaments of dust emission in intricate detail. We present a pilot study to …

Observations of pulsar scintillation are among the few astrophysical probes of very small-
scale (≲ au) phenomena in the interstellar medium (ISM). In particular, characterization of …

Context. Despite recent observational and theoretical advances in mapping the magnetic
fields associated with molecular clouds, their three-dimensional (3D) morphology remains …

Our Sun lies within 300 parsecs of the 2.7-kiloparsecs-long sinusoidal chain of dense gas
clouds known as the Radcliffe Wave. The structure's wave-like shape was discovered using …

Knowledge of the three-dimensional structure of Galactic molecular clouds is important for
understanding how clouds are affected by processes such as turbulence and magnetic …

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 …

Context. Measurements of long-lived radioisotopes, which have grown rapidly in quantity
and sensitivity over the last few years, provide a means, completely independent of other …

We present the first Bayesian method for tomographic decomposition of the plane-of-sky
orientation of the magnetic field with the use of stellar polarimetry and distance. This …