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Radio Study of the Pulsar Wind Nebula Powered by PSR B1706-44
Y. H. Liu, C. Y. Ng,
R. Dodson
International Centre for Radio Astronomy Research (ICRAR)
Research output
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Contribution to journal
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Article
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peer-review
1
Citation (Scopus)
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Physics
Pulsar
100%
Nebula
100%
X Ray
37%
Supernova Remnant
25%
Gamma Radiation
12%
Radio Pulsars
12%
Energetics
12%
Magnetic Field
12%
Supernovae
12%
Deceleration
12%
Radio Spectra
12%
Radio Emission
12%