activity
20212026
most citedEvidence for Line-of-Sight Frequency Decorrelation of Polarized Dust Emission in Data

53 citations · 53 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

LightCube: A Parsec-Resolution 3D Model of the Local Far-Ultraviolet Interstellar Radiation Field

Hannah V. Bish, J. E. G. Peek, Catherine Zucker +5

We present a three-dimensional model of the local interstellar radiation field (ISRF) in the ultraviolet (UV). Using UV flux measurements from the TD1 catalog and stellar distances…

astro-ph.GA2026

The Multi-phase HI of the Milky Way and Nearby Galaxies

Marc-Antoine Miville-Deschênes, J. R. Dawson, Narendra Nath Patra +30

Atomic hydrogen (HI) is the dominant baryonic component of the interstellar medium (ISM) in Milky Way-like galaxies and the reservoir from which molecular clouds and stars ultimate…

astro-ph.GA2026

Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect

Timothy Robishaw, Marta Nowotka, Tao-Chung Ching +7

Zeeman splitting in spectral lines -- both in emission and absorption -- provides direct estimates of magnetic field strength and direction in magnetized gas in our own Milky Way a…

astro-ph.GA2026

Far-infrared Polarization Properties of Nearby Star-forming Regions: A New Compendium of SOFIA/HAWC+ Observations

Kaitlyn Karpovich, Susan E. Clark, Enrique Lopez-Rodriguez

We present a comprehensive polarimetric study of 26 nearby molecular clouds in four far-infrared bands (53 m~to 214~m) using 52 archival SOFIA/HAWC+ datasets{, over half of w…

astro-ph.GA2025

Joint Analysis of HI Absorption Zeeman Measurements and the Morphology of Filamentary HI Emission

Marta Nowotka, Susan E. Clark, Blakesley Burkhart +4

We present a joint analysis of HI absorption Zeeman measurements and the morphology of filamentary HI emission to investigate the three-dimensional structure of the magnetic field…

astro-ph.GA2024

Tracing 3-D Magnetic Field Structure Using Dust Polarization and the Zeeman Effect

Brandon Shane, Blakesley Burkhart, Laura Fissel +3

The characterization of magnetic fields within molecular clouds is fundamental to understanding star formation processes. Accurately gauging the three-dimensional structure of thes…

astro-ph.CO2021★ 53 cited

Evidence for Line-of-Sight Frequency Decorrelation of Polarized Dust Emission in Data

V. Pelgrims, S. E. Clark, B. S. Hensley +5

If a single line of sight (LOS) intercepts multiple dust clouds of different spectral energy distributions and magnetic field orientations, the frequency scaling of each of the Sto…