We present a new three-dimensional map of dust reddening, based on Gaia parallaxes and
stellar photometry from Pan-STARRS 1 and 2MASS. This map covers the sky north of a decl …

Context. The third Gaia data release (Gaia DR3) contains, beyond the astrometry and
photometry, dispersed light for hundreds of millions of sources from the Gaia prism spectra …

Aims. Mapping the interstellar medium in 3D provides a wealth of insights into its inner
working. The Milky Way is the only galaxy for which detailed 3D mapping can be achieved in …

We leverage the 1 pc spatial resolution of the Leike et al. three-dimensional (3D) dust map
to characterize the 3D structure of nearby molecular clouds (d≲ 400 pc). We start by" …

A major question in the field of star formation is how molecular clouds form out of the diffuse
interstellar medium (ISM). Recent advances in 3D dust mapping are revolutionizing our view …

Galaxies are observed to host magnetic fields with a typical total strength of around 15 μ G.
A coherent large-scale field constitutes up to a few microgauss of the total, while the rest is …

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 …

The Sun is embedded in the so-called Local Bubble (LB)–a cavity of hot plasma created by
supernova explosions and surrounded by a shell of cold, dusty gas. Knowing the local …

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 …