A Persistent Disk Wind and Variable Jet Outflow in the Neutron-star Low-mass X-Ray Binary GX 13+1 Article Swipe
YOU?
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· 2025
· Open Access
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· DOI: https://doi.org/10.3847/1538-4357/adcabe
In low-mass X-ray binaries (LMXBs), accretion flows are often associated with either jet outflows or disk winds. Studies of LMXBs with luminosities up to roughly 20% of the Eddington limit indicate that these outflows generally do not co-occur, suggesting that disk winds might inhibit jets. However, previous observations of LMXBs accreting near or above the Eddington limit show that jets and winds can potentially coexist. To investigate this phenomenon, we carried out a comprehensive multiwavelength campaign (using the Very Large Array (VLA), Chandra/High Energy Transmission Grating Spectrometer (HETG), and NICER) on the near-Eddington neutron-star Z-source LMXB GX 13+1. NICER and Chandra/HETG observations tracked GX 13+1 across the entire Z track during high Eddington rates, detecting substantial resonance absorption features originating from the accretion disk wind in all X-ray spectra, which implies a persistent wind presence. Simultaneous VLA observations captured a variable radio jet, with radio emission notably strong during all flaring branch observations—contrary to typical behavior in Z sources—and weaker when the source was on the normal branch. Interestingly, no clear correlation was found between the radio emission and the wind features. Analysis of VLA radio light curves and simultaneous Chandra/HETG spectra demonstrates that an ionized disk wind and jet outflow can indeed coexist in GX 13+1, suggesting that their launching mechanisms are not necessarily linked in this system.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/adcabe
- OA Status
- gold
- Cited By
- 1
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- OpenAlex ID
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Raw OpenAlex JSON
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https://openalex.org/W4411033126Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/adcabeDigital Object Identifier
- Title
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A Persistent Disk Wind and Variable Jet Outflow in the Neutron-star Low-mass X-Ray Binary GX 13+1Work title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-06-04Full publication date if available
- Authors
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Daniele Rogantini, J. Homan, Richard M. Plotkin, M. van den Berg, J. C. A. Miller‐Jones, Joey Neilsen, Deepto Chakrabarty, R. P. Fender, Norbert S. SchulzList of authors in order
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https://doi.org/10.3847/1538-4357/adcabePublisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/adcabeDirect OA link when available
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Physics, Astrophysics, X-ray binary, Neutron star, Outflow, X-ray burster, Astronomy, Jet (fluid), Binary number, Binary star, Stellar mass loss, Stellar evolution, Mechanics, Stars, Arithmetic, Mathematics, MeteorologyTop concepts (fields/topics) attached by OpenAlex
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1Total citation count in OpenAlex
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2025: 1Per-year citation counts (last 5 years)
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103Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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