output
20142025
most citedThe Galactic Magneto-Ionic Medium Survey: Moments of the Faraday Spectra

46 citations

Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA202129 cited

The Global Magneto-Ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280-1750 MHz

M. Wolleben, T. L. Landecker, K. A. Douglas +17

The Galactic interstellar medium hosts a significant magnetic field, which can be probed through the synchrotron emission produced from its interaction with relativistic electrons.…

astro-ph.GA202119 cited

Revisiting Rotation Measures from the Canadian Galactic Plane Survey: the Magnetic Field in the Disk of the Outer Galaxy

C. L. Van Eck, J. C. Brown, A. Ordog +9

Faraday rotation provides a valuable tracer of magnetic fields in the interstellar medium; catalogs of Faraday rotation measures provide key observations for studies of the Galacti…

astro-ph.GA201846 cited

The Galactic Magneto-Ionic Medium Survey: Moments of the Faraday Spectra

John M. Dickey, T. L. Landecker, A. J. M. Thomson +11

Faraday rotation occurs along every line of sight in the Galaxy; Rotation Measure (RM) synthesis allows a three-dimensional representation of the interstellar magnetic field. This…

astro-ph.GA201727 cited

The Fan Region at 1.5 GHz. I: Polarized synchrotron emission extending beyond the Perseus Arm

A. S. Hill, T. L. Landecker, E. Carretti +12

The Fan Region is one of the dominant features in the polarized radio sky, long thought to be a local (distance < 500 pc) synchrotron feature. We present 1.3-1.8 GHz polarized radi…

astro-ph.GA201613 cited

A High-Velocity Cloud Impact Forming a Supershell in the Milky Way

Geumsook Park, Bon-Chul Koo, Ji-hyun Kang +5

Neutral atomic hydrogen (HI) gas in interstellar space is largely organized into filaments, loops, and shells, the most prominent of which are "supershells". These gigantic structu…

astro-ph.GA20147 cited

The Emission Nebula Sh 2-174: A Radio Investigation of the Surrounding Region

R. R. Ransom, R. Kothes, J. Geisbuesch +2

Sh 2-174 is believed to be either a planetary nebula (PN) or ionized, ambient interstellar medium (ISM). We present in this paper 1420 MHz polarization, 1420 MHz total intensity (S…