## 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

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

Supersonic isothermal turbulence establishes a network of transient dense shocks that sweep up material and have a density profile described by balance between ram pressure of the background fluid versus

## Thomson et al. (2018) – Ghost of a shell: magnetic fields of Galactic supershell GSH 006 – 15 + 7

We identify a counterpart to a Galactic supershell in diffuse radio polarization, and use this to determine the magnetic fields associated with this object. GSH 006 – 15 + 7

## 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

## 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

## 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

## 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

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

The Galactic neutral hydrogen (H I ) sky at high Galactic latitudes is suffused with linear structure. Particularly prominent in narrow spectral intervals, these linear H I features are well

## 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

We compare the magnetic field orientation for the young giant molecular cloud Vela C inferred from 500-$\mu$m polarization maps made with the BLASTPol balloon-borne polarimeter to the orientation of structures