New MeerKAT images reveal diffuse radio emission inside SNR G338.3-0.0, likely the radio sign of a pulsar wind nebula that may be feeding cosmic-ray electrons into the Galaxy.
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Detection of Diffuse Radio Emission inside the Supernova Remnant G338.3-0.0 associated with the Gamma-ray Source HESS J1640-465
New MeerKAT images reveal diffuse radio emission inside SNR G338.3-0.0, likely the radio sign of a pulsar wind nebula that may be feeding cosmic-ray electrons into the Galaxy.