HI absorption is detected in three sight lines through two disk galaxies at 7-22 Mpc, yielding Local-Group-like spin temperatures but lower CNM fractions due to resolution averaging in emission spectra.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 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
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HI absorption in MHONGOOSE -- Spin temperatures and cold neutral medium in nearby disk galaxies
HI absorption is detected in three sight lines through two disk galaxies at 7-22 Mpc, yielding Local-Group-like spin temperatures but lower CNM fractions due to resolution averaging in emission spectra.
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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.