## Tchernyshyov, Peek & Zasowski (2018) – Kinetic Tomography. II. A Second Method for Mapping the Velocity Field of the Milky Way Interstellar Medium and a Comparison with Spiral Structure Models

In this work, we derive a spatially resolved map of the line-of-sight velocity of the interstellar medium and use it, along with a second map of line-of-sight velocity from Paper

## Alig et al. (2018) – Simulating the Impact of the Smith Cloud

We investigate the future evolution of the Smith Cloud by performing hydrodynamical simulations of the cloud impact onto the gaseous Milky Way Galactic disk. We assume a local origin for

## Putman, Peek & Joung (2012) – Gaseous Galaxy Halos

Galactic halo gas traces inflowing star-formation fuel and feedback from a galaxy’s disk and is therefore crucial to our understanding of galaxy evolution. In this review, we summarize the multiwavelength

## Mattern et al. (2018) – SEDIGISM: The kinematics of ATLASGAL filaments

Analysing the kinematics of filamentary molecular clouds is a crucial step towards understanding their role in the star formation process. Therefore, we study the kinematics of 283 filament candidates in

## van de Hulst, Muller & Oort (1954) – The spiral structure of the outer part of the Galactic System derived from the hydrogen emission at 21 cm wavelength

Not Available van de Hulst, H. C.; Muller, C. A.; Oort, J. H. 1954, Bulletin of the Astronomical Institutes of the Netherlands, 12, 117 http://cdsads.u-strasbg.fr/abs/1954BAN….12..117V

## Heiles (1982) – Temperatures and their variation within interstellar H I structures

Recent H I absorption surveys are used to derive H I temperatures T(H I) and their variation within a number of H I shells. In these shells T(H I) is

## Palouš & Ehlerová (2017) – Gould’s Belt: Local Large-Scale Structure in the Milky Way

Gould’s Belt is a flat local system composed of young massive stars of spectral types O or early-type B (OB stars), molecular clouds, and neutral hydrogen within 500 pc of

## Ramón-Fox & Bonnell (2018) – Streaming motions and kinematic distances to molecular clouds

We present high-resolution smoothed particle hydrodynamics simulations of a region of gas flowing in a spiral arm and identify dense gas clouds to investigate their kinematics with respect to a