Radio Study of the Pulsar Wind Nebula Powered by PSR B1706-44

Radio Study of the Pulsar Wind Nebula Powered by PSR B1706-44

PSR B1706−44 is an energetic gamma-ray pulsar located inside supernova remnant (SNR) G343.1−2.3 and it powers a compact pulsar wind nebula (PWN) that shows torus and jet structure in X-rays. We present a radio study of the PWN using Australia Telescope Compact Array observations at 3, 6, 13, and 21...

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Bibliographic Details
Main Authors: Y. H. Liu, C.-Y. Ng, R. Dodson
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Pulsar wind nebulae
Supernova remnants
Polarimetry
Online Access:https://doi.org/10.3847/1538-4357/acb20d

Internet

https://doi.org/10.3847/1538-4357/acb20d

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