New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2representative citing papers
Stacking Stokes Q and U cubes from 27 galaxies reveals an X-shaped polarization pattern extending 9 kpc into the halo, with ~60% PI drop near the minor axis, stronger emission on the approaching side, and 90 rad m^{-2} systematic RM uncertainty, but no confirmed global RM pattern.
citing papers explorer
-
A new wideband radio polarization observation of the Supernova Remnant G315.4$-$2.3
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.
-
CHANG-ES XXXIX. Magnetic field structure in edge-on galaxies: Stacking Stokes parameters
Stacking Stokes Q and U cubes from 27 galaxies reveals an X-shaped polarization pattern extending 9 kpc into the halo, with ~60% PI drop near the minor axis, stronger emission on the approaching side, and 90 rad m^{-2} systematic RM uncertainty, but no confirmed global RM pattern.