Curtin University Homepage
  • Library
  • Help
    • Admin

    espace - Curtin’s institutional repository

    JavaScript is disabled for your browser. Some features of this site may not work without it.
    View Item 
    • espace Home
    • espace
    • Curtin Research Publications
    • View Item
    • espace Home
    • espace
    • Curtin Research Publications
    • View Item

    A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597-3704, in the Globular Cluster NGC 6256

    265471.pdf (734.1Kb)
    67689.pdf (1.758Mb)
    Access Status
    Open access
    Authors
    Tetarenko, A.
    Bahramian, A.
    Wijnands, R.
    Heinke, C.
    Maccarone, T.
    Miller-Jones, James
    Strader, J.
    Chomiuk, L.
    Degenaar, N.
    Sivakoff, G.
    Altamirano, D.
    Deller, A.
    Kennea, J.
    Li, K.
    Plotkin, Richard
    Russell, T.
    Shaw, A.
    Date
    2018
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Tetarenko, A. and Bahramian, A. and Wijnands, R. and Heinke, C. and Maccarone, T. and Miller-Jones, J. and Strader, J. et al. 2018. A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597-3704, in the Globular Cluster NGC 6256. Astrophysical Journal. 854: article number 2.
    Source Title
    Astrophysical Journal
    DOI
    10.3847/1538-4357/aaa95a
    ISSN
    0004-637X
    School
    Curtin Institute of Radio Astronomy (Physics)
    Funding and Sponsorship
    http://purl.org/au-research/grants/arc/FT140101082
    Remarks

    Copyright © 2018 The American Astronomical Society. All rights reserved.

    URI
    http://hdl.handle.net/20.500.11937/67507
    Collection
    • Curtin Research Publications
    Abstract

    We present Karl G. Jansky Very Large Array radio frequency observations of the new accreting millisecond X-ray pulsar (AMXP), IGR J16597-3704, located in the globular cluster NGC 6256. With these data, we detect a radio counterpart to IGR J16597-3704, and determine an improved source position. Pairing our radio observations with quasi-simultaneous Swift/XRT X-ray observations, we place IGR J16597-3704 on the radio-X-ray luminosity plane, where we find that IGR J16597-3704 is one of the more radio-quiet neutron star low-mass X-ray binaries known to date. We discuss the mechanisms that may govern radio luminosity (and in turn jet production and evolution) in AMXPs. Furthermore, we use our derived radio position to search for a counterpart in archival Hubble Space Telescope and Chandra X-ray Observatory data, and estimate an upper limit on the X-ray luminosity of IGR J16597-3704 during quiescence.

    Related items

    Showing items related by title, author, creator and subject.

    • Radio and X-ray variability in the Seyfert galaxy NGC 4051
      Jones, S.; McHardy, I.; Moss, D.; Seymour, Nick; Breedt, E.; Uttley, P.; Körding, E.; Tudose, V. (2011)
      We present intensive quasi-simultaneous X-ray and radio monitoring of the narrow line Seyfert 1 galaxy NGC 4051, over a 16-month period in 2000–01. The X-ray observations were made with the Proportional Counter Array on ...
    • Linking Jet Emission, X-Ray States, and Hard X-Ray Tails in the Neutron Star X-Ray Binary GX 17+2
      Migliari, S.; Miller-Jones, James; Fender, R.; Homan, J.; Di Salvo, T.; Rothschild, R.; Rupen, M.; Tomsick, J.; Wijnands, R.; van der Klis, M. (2007)
      We present the results of simultaneous radio (VLA) and X-ray (RXTE) observations of the Z-type neutron star X-ray binary GX 17+2. The aim is to assess the coupling between X-ray and radio properties throughout its three ...
    • Radio observations of the merging galaxy cluster Abell 520
      Hoang, D.N.; Shimwell, T.W.; Van Weeren, R.J.; Brunetti, G.; Röttgering, H.J.A.; Andrade-Santos, F.; Botteon, A.; Brüggen, M.; Cassano, R.; Drabent, A.; De Gasperin, F.; Hoeft, M.; Intema, Huib ; Rafferty, D.A.; Shweta, A.; Stroe, A. (2019)
      Context. Extended synchrotron radio sources are often observed in merging galaxy clusters. Studies of the extended emission help us to understand the mechanisms in which the radio emitting particles gain their relativistic ...
    Advanced search

    Browse

    Communities & CollectionsIssue DateAuthorTitleSubjectDocument TypeThis CollectionIssue DateAuthorTitleSubjectDocument Type

    My Account

    Admin

    Statistics

    Most Popular ItemsStatistics by CountryMost Popular Authors

    Follow Curtin

    • 
    • 
    • 
    • 
    • 

    CRICOS Provider Code: 00301JABN: 99 143 842 569TEQSA: PRV12158

    Copyright | Disclaimer | Privacy statement | Accessibility

    Curtin would like to pay respect to the Aboriginal and Torres Strait Islander members of our community by acknowledging the traditional owners of the land on which the Perth campus is located, the Whadjuk people of the Nyungar Nation; and on our Kalgoorlie campus, the Wongutha people of the North-Eastern Goldfields.