CR-MHD simulations of a Milky Way analogue reproduce observed gamma-ray luminosities and spectra without tuning, with sky morphology set by local gas density fluctuations and angular power spectra tracing gas column rather than cosmic-ray density.
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A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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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The diffuse gamma-ray sky of a Milky Way analogue: Local diversity and global constraints
CR-MHD simulations of a Milky Way analogue reproduce observed gamma-ray luminosities and spectra without tuning, with sky morphology set by local gas density fluctuations and angular power spectra tracing gas column rather than cosmic-ray density.
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Multiwavelength Probes of Cosmic Ray Transport in Molecular Cloud Structures
A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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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.