## Green et al. (2019) – A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS

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 declination

## Clark, Peek & Miville-Deschênes (2019) – The Physical Nature of Neutral Hydrogen Intensity Structure

We investigate the physical properties of structures seen in channel map observations of 21 cm neutral hydrogen (H I) emission. H I intensity maps display prominent linear structures that are

## Panopoulou et al. (2019) – Extreme starlight polarization in a region with highly polarized dust emission

Context. Galactic dust emission is polarized at unexpectedly high levels, as revealed by Planck. Aims: The origin of the observed ~=20% polarization fractions can be identified by characterizing the properties

## Zucker et al. (2019) – A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition

We present a uniform catalog of accurate distances to local molecular clouds informed by the Gaia DR2 data release. Our methodology builds on that of Schlafly et al. (2014). First,

## Fukui et al. (2018) – Synthetic Observations of 21 cm H I Line Profiles from Inhomogeneous Turbulent Interstellar H I Gas with Magnetic Fields

We carried out synthetic observations of interstellar atomic hydrogen at 21 cm wavelength by utilizing the magnetohydrodynamic numerical simulations of the inhomogeneous turbulent interstellar medium. The cold neutral medium (CNM)

## Galliano (2018) – A dust spectral energy distribution model with hierarchical Bayesian inference – I. Formalism and benchmarking

This article presents a new dust spectral energy distribution (SED) model, named HerBIE, aimed at eliminating the noise-induced correlations and large scatter obtained when performing least-squares fits. The originality of

## Cortese et al. (2010) – Diffuse far-infrared and ultraviolet emission in the NGC 4435/4438 system: tidal stream or Galactic cirrus?

We report the discovery of diffuse far-infrared and far-ultraviolet emission projected near the interacting pair NGC 4435/4438, in the Virgo cluster. This feature spatially coincides with a well-known low surface-brightness

## Liu, von Hausegger & Naselsky (2017) – Towards understanding the Planck thermal dust models

Understanding the properties of dust emission in the microwave domain is an important premise for the next generation of cosmic microwave background (CMB) experiments, devoted to the measurement of the

## Chiang & Ménard (2018) – Extragalactic Imprints in Galactic Dust Maps

Extragalactic astronomy relies on the accurate estimation of source photometry corrected for Milky Way dust extinction. This has motivated the creation of a number of “Galactic” dust maps. We investigate

## Liszt (2014) – N(H I)/E(B – V)

We explore the relationship between dust-emission derived reddening E(B – V) and atomic hydrogen column density N(H I) derived from 21 cm emission surveys. We consider measurements at galactic latitudes

## Reach et al. (2017) – Variations between Dust and Gas in the Diffuse Interstellar Medium. III. Changes in Dust Properties

We study infrared emission of 17 isolated, diffuse clouds with masses of order {10}2 {M}&sun; to test the hypothesis that grain property variations cause the apparently low gas-to-dust ratios that

## Ysard et al. (2018) – The optical properties of dust: the effects of composition, size, and structure

Grains are determinant for setting the chemical, physical, dynamical, and radiative properties of all the media in which they are present. Their influence depends on the grain composition, size, and

## Skalidis et al. (2018) – Local measurements of the mean interstellar polarization at high Galactic latitudes

Very little information exists concerning the properties of the interstellar medium (ISM)-induced starlight polarization at high Galactic latitudes. Future optopolarimetric surveys promise to fill this gap. We conduct a small-scale

## McKinnon et al. (2018) – Simulating galactic dust grain evolution on a moving mesh

Interstellar dust is an important component of the galactic ecosystem, playing a key role in multiple galaxy formation processes. We present a novel numerical framework for the dynamics and size

## Jokipii, Lerche & Schommer (1969) – Interstellar Polarization of Starlight and the Turbulent Structure of the Galaxy

Fluctuations in the polarization of starlight provide strong support for the concept of a turbulent interstellar medium. We have analyzed theoretically the mean polarization and the variance of polarization about

## Aannestad & Purcell (1973) – Interstellar Grains

Not Available Aannestad, Per A.; Purcell, Edward M. 1973, Annual Review of Astronomy and Astrophysics, 11, 309 http://adsabs.harvard.edu/abs/1973ARA%26A..11..309A

## Zucker, Battersby & Goodman (2018) – The Physical Properties of Large-Scale Galactic Filaments

The characterization of our Galaxy’s longest filamentary gas features has been the subject of several studies in recent years, producing not only a sizeable sample of large-scale filaments, but also

## Papoular (2018) – A new interpretation of Serkowski’s polarization law

The basic tenets of the alternative interpretation to be presented here are that the spectral profiles of the star light polarization peaks observed in the visible and near IR are

## Ivlev et al. (2018) – Compact Dusty Clouds and Efficient H2 Formation in Diffuse Interstellar Medium

The formation of compact dusty clouds in diffuse interstellar medium (ISM) has been recently proposed and studied by Tsytovich et al. In the present paper, the effect of the clouds

## Juvela et al. (2018) – Galactic cold cores. IX. Column density structures and radiative-transfer modelling

Context. The Galactic Cold Cores (GCC) project has made Herschel photometric observations of interstellar clouds where Planck detected compact sources of cold dust emission. The fields are in different environments

## Murray et al. (2018) – Optically Thick H I Does Not Dominate Dark Gas in the Local ISM

The local interstellar medium (ISM) is suffused with “dark” gas, identified by excess infrared and gamma-ray emission, yet undetected by standard ISM tracers such as neutral hydrogen (H I) or

## Nguyen et al. (2018) – Dust-Gas Scaling Relations and OH Abundance in the Galactic ISM

Observations of interstellar dust are often used as a proxy for total gas column density N H. By comparing Planck thermal dust data (Release 1.2) and new dust reddening maps

## Planck Collaboration et al. (2018) – Planck 2018 results. XII. Galactic astrophysics using polarized dust emission

We present 353 GHz full-sky maps of the polarization fraction $p$, angle $\psi$, and dispersion of angles $S$ of Galactic dust thermal emission produced from the 2018 release of Planck