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A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597-3704, in the Globular Cluster NGC 6256
A. J. Tetarenko
, A. Bahramian
, R. Wijnands
, C. O. Heinke
, T. J. Maccarone
, J. C.A. Miller-Jones
, J. Strader
, L. Chomiuk
, N. Degenaar
, G. R. Sivakoff
, D. Altamirano
, A. T. Deller
,
J. A. Kennea
, K. L. Li
, R. M. Plotkin
, T. D. Russell
, A. W. Shaw
Astronomy & Astrophysics
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Article
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peer-review
13
Scopus citations
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Keyphrases
Radio Frequency
100%
Radio
100%
Globular Clusters
100%
X-ray Pulsar
100%
Luminosity
60%
X-ray
40%
X-ray Observations
20%
Neutron Stars
20%
Hubble Space Telescope
20%
Swift
20%
Frequency Estimation
20%
Quiescence
20%
Chandra X-ray Observatory
20%
Very Large Array
20%
Source Position
20%
Radio Observations
20%
Jet Production
20%
Low-mass X-ray Binaries
20%
Observatory Data
20%
Jet Evolution
20%
Improved Source
20%
Physics
X Ray
100%
Pulsar
100%
Globular Cluster
100%
Neutron Stars
20%
Hubble Space Telescope
20%
X-Ray Observatories
20%
Very Large Array
20%
Low-Mass X-Ray Binary Stars
20%