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Radio Harps in the Galactic Center: A Laboratory for Cosmic-Ray Transport

Radio observations of the Galactic center reveal striking filaments of synchrotron emission, formed as cosmic ray (CR) electrons travel along magnetic fields. Researchers tested different CR transport models and found that a combination of diffusion and streaming best explains the observed filament structures. This study not only sheds light on how CRs move through space but also provides a new way to probe the magnetic environment of our galaxy.

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