interstellar

Thompson, Troland & Heiles (2019) – A Survey of Magnetic Field Strengths in the Envelopes of Molecular Clouds via the 18 cm OH Zeeman Effect

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

Peek & Burkhart (2019) – Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium

Marchal et al. (2019) – ROHSA: Regularized Optimization for Hyper-Spectral Analysis – Application to phase separation of 21 cm data

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

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

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

Heiles et al. (2019) – The interstellar medium: the key component in galactic evolution and modern cosmology

González-Casanova, Lazarian & Burkhart (2019) – Velocity centroid gradients for absorbing media

Körtgen, Federrath & Banerjee (2019) – On the shape and completeness of the column density probability distribution function of molecular clouds

Hanany et al. (2019) – PICO: Probe of Inflation and Cosmic Origins

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

Mocz & Burkhart (2018) – Star formation from dense shocked regions in supersonic isothermal magnetoturbulence

Körtgen et al. (2018) – The Origin of Filamentary Star Forming Clouds in Magnetised Galaxies

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

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

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

Clark (2018) – A New Probe of Line-of-sight Magnetic Field Tangling

Fissel et al. (2018) – Relative Alignment Between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud using Low and High Density Tracers

Li et al. (2018) – Where is OH and Does It Trace the Dark Molecular Gas (DMG)?

Körtgen, Federrath & Banerjee (2017) – The driving of turbulence in simulations of molecular cloud formation and evolution