Associating LOFAR Galactic Faraday structures with the warm neutral medium
F. Boulanger, C. Gry, E. B. Jenkins, A. Bracco, A. Erceg, V. Jeli\'c, and L. Turi\'c

TL;DR
This study links LOFAR-detected Faraday structures with the warm neutral medium in the ISM by combining multi-wavelength data, revealing a magnetized WNM slab ahead of the warm ionized medium, and establishing a framework for future ISM studies.
Contribution
It introduces a method to associate LOFAR Faraday structures with the warm neutral medium using UV, dust polarization, and magnetic field modeling, advancing understanding of the magnetized ISM.
Findings
LOFAR structures trace a magnetized WNM slab.
The WNM slab is located ahead of the warm ionized medium.
The study provides a framework for future ISM magnetic field research.
Abstract
Faraday tomography observations with the Low Frequency Array (LOFAR) have unveiled a remarkable network of structures in polarized synchrotron emission at high Galactic latitudes. The observed correlation between LOFAR structures, dust polarization, and HI emission suggests a connection to the neutral interstellar medium (ISM). We investigated this relationship by estimating the rotation measure (RM) of the warm neutral (partially ionized) medium (WNM) in the local ISM. Our work combines UV spectroscopy from FUSE and dust polarization observations from \Planck\ with LOFAR data. We derived electron column densities from UV absorption spectra toward nine background stars, within the field of published data from the LOFAR two-meter sky survey. The associated RMs were estimated using a local magnetic field model fitted to the dust polarization data of \Planck. A comparison with Faraday…
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