Rotation measure synthesis at the 2 m wavelength of the FAN region: Unveiling screens and bubbles
Marco Iacobelli (1,2), Marijke Haverkorn (3,1), Peter Katgert (1), ((1) Leiden University, (2) ASTRON, the Netherlands Institute for Radio, Astronomy, (3) Radboud University Nijmegen)

TL;DR
This study uses rotation measure synthesis at 2m wavelength to reveal and analyze complex magnetic and ionized structures in the interstellar medium of the FAN region, identifying features like the Local Bubble wall and a potential relic Stromgren sphere.
Contribution
First application of cross-correlation in Faraday depth space to characterize polarized structures, revealing new insights into interstellar magnetic field morphology and turbulence.
Findings
Detection of magnetic field reversal along the line of sight.
Identification of structures associated with the Local Bubble wall.
Evidence of turbulence in polarized structures.
Abstract
Rotation Measure synthesis (RM synthesis) of the Westerbork Synthesis Radio Telescope (WSRT) observations at 2 m wavelength of the FAN region at l=137deg, b=+7deg shows the morphology of structures in the ionized interstellar medium. We interpret the diffuse polarized synchrotron emission in terms of coherent structures in the interstellar medium and the properties of the interstellar magnetic field. For the first time, cross-correlation is applied to identify and characterize polarized structures in Faraday depth space. Complementary information about the medium are derived from H emission, properties of nearby pulsars, and optical polarized starlight measurements. Three morphological patterns are recognized, showing structures on scales from degrees down to the beam size. At low Faraday depth values, a low gradient across the imaged field is detected, almost aligned with the…
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