uGMRT at 736 and 1274 MHz reveals an elongated radio counterpart to the X-ray PWN of PSR J2030+4415, with spectral index variations and restrictive upper limits on the pulsar and filament.
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Exploring the non-thermal physics behind the pulsar wind nebula PSR J2030+4415 through radio observations
uGMRT at 736 and 1274 MHz reveals an elongated radio counterpart to the X-ray PWN of PSR J2030+4415, with spectral index variations and restrictive upper limits on the pulsar and filament.