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

The unprecedented quality of the astrometric measurements obtained with the ESA Gaia
spacecraft have initiated a revolution in Milky Way astronomy. Studies of star clusters in …

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 …

Aims. Three-dimensional (3D) maps of Galactic interstellar dust are a tool for a wide range of
uses. We aim to construct 3D maps of dust extinction in the Local Arm and surrounding …

The last decade of direct imaging (DI) searches for sub-stellar companions has uncovered a
widely diverse sample that challenges the current formation models, while highlighting the …

Context. Three-dimensional (3D) maps of the extinction density in the Milky Way can be built
through the inversion of large catalogues of distance-extinction pairs for individual target …

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" …

While astrophysical and cosmological probes provide a remarkably precise and consistent
picture of the quantity and general properties of dark matter, its fundamental nature remains …

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 …

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 …