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The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8−1613

The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8−1613
The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8−1613
Tracking the correlation between radio and X-ray luminosities during black hole X-ray binary outbursts is a key diagnostic of the coupling between accretion inflows (traced by X-rays) and relativistic jet outflows (traced by radio). We present the radio–X-ray correlation of the black hole low-mass X-ray binary Swift J1727.8−1613 during its 2023–2024 outburst. Our observations span a broad dynamic range, covering ∼4 orders of magnitude in radio luminosity and ∼6.5 in X-ray luminosity. This source follows an unusually radio-quiet track, exhibiting significantly lower radio luminosities at a given X-ray luminosity than both the standard (radio-loud) track and most previously known radio-quiet systems. Across most of the considered distance range(D ∼ 1.5–4.3 kpc), Swift J1727.8−1613 appears to be the most radio-quiet black hole binary identified to date. For distances≥ 4 kpc, while Swift J1727 becomes comparable to one other extremely radio-quiet system, its peak X-ray luminosity (≥ 5×1038erg s−1) exceeds that of any previously reported hard-state black hole low-mass X-ray binary, emphasizing the extremity of this outburst. Additionally, for the first time in a radio-quiet system, we identify the onset of X-ray spectral softening to coincide with a change in trajectory through the radio–X-ray plane. We assess several proposed explanations for radio-quiet behaviour in black hole systems in light of this data set. As with other such sources, however, no single mechanism fully accounts for the observed properties, highlighting the importance of regular monitoring and the value of comprehensive (quasi-)simultaneous data-sets
astro-ph.HE
1365-2966
1803–1816
Hughes, A.K.
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Carotenuto, F.
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Russell, T.D.
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Tetarenko, A.J.
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Miller-Jones, J.C.A.
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Plotkin, R.M.
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Bahramian, A.
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Bright, J.S.
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Cowie, F.J.
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Crook-Mansour, J.
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Fender, R.
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Khaulsay, J.K.
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Kirby, A.
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Jones, S.
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McCollough, M.
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Rao, R.
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Sivakoff, G.R.
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Vrtilek, S.D.
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Williams-Baldwin, D.R.A.
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Wood, C.M.
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Altamirano, D.
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Casella, P.
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Segura, N. Castro
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Corbel, S.
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Santo, M. Del
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Echiburu-Trujillo, C.
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van den Eijnden, J.
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Gallo, E.
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Gandhi, P.
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Koljonen, K.I.I.
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Maccarone, T.
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Markoff, S.B.
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Motta, S.
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Russell, D.M.
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Saikia, P.
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Shaw, A.W.
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Soria, R.
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Tomsick, J.A.
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Yu, W.
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et al.
Hughes, A.K.
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Carotenuto, F.
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Russell, T.D.
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Tetarenko, A.J.
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Miller-Jones, J.C.A.
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Bahramian, A.
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Bright, J.S.
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Cowie, F.J.
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Fender, R.
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Jones, S.
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Rao, R.
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Sivakoff, G.R.
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Vrtilek, S.D.
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Altamirano, D.
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Casella, P.
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Segura, N. Castro
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Corbel, S.
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Santo, M. Del
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Echiburu-Trujillo, C.
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van den Eijnden, J.
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Gallo, E.
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Gandhi, P.
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Koljonen, K.I.I.
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Maccarone, T.
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Markoff, S.B.
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Motta, S.
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Russell, D.M.
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Saikia, P.
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Shaw, A.W.
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Soria, R.
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Tomsick, J.A.
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Yu, W.
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Zhang, X.
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Hughes, A.K., Carotenuto, F. and Russell, T.D. , et al. (2025) The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8−1613. Monthly Notices of the Royal Astronomical Society, 542 (3), 1803–1816. (doi:10.1093/mnras/staf1363).

Record type: Article

Abstract

Tracking the correlation between radio and X-ray luminosities during black hole X-ray binary outbursts is a key diagnostic of the coupling between accretion inflows (traced by X-rays) and relativistic jet outflows (traced by radio). We present the radio–X-ray correlation of the black hole low-mass X-ray binary Swift J1727.8−1613 during its 2023–2024 outburst. Our observations span a broad dynamic range, covering ∼4 orders of magnitude in radio luminosity and ∼6.5 in X-ray luminosity. This source follows an unusually radio-quiet track, exhibiting significantly lower radio luminosities at a given X-ray luminosity than both the standard (radio-loud) track and most previously known radio-quiet systems. Across most of the considered distance range(D ∼ 1.5–4.3 kpc), Swift J1727.8−1613 appears to be the most radio-quiet black hole binary identified to date. For distances≥ 4 kpc, while Swift J1727 becomes comparable to one other extremely radio-quiet system, its peak X-ray luminosity (≥ 5×1038erg s−1) exceeds that of any previously reported hard-state black hole low-mass X-ray binary, emphasizing the extremity of this outburst. Additionally, for the first time in a radio-quiet system, we identify the onset of X-ray spectral softening to coincide with a change in trajectory through the radio–X-ray plane. We assess several proposed explanations for radio-quiet behaviour in black hole systems in light of this data set. As with other such sources, however, no single mechanism fully accounts for the observed properties, highlighting the importance of regular monitoring and the value of comprehensive (quasi-)simultaneous data-sets

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Accepted/In Press date: 14 June 2025
e-pub ahead of print date: 19 August 2025
Published date: 29 August 2025
Keywords: astro-ph.HE

Identifiers

Local EPrints ID: 506750
URI: http://eprints.soton.ac.uk/id/eprint/506750
ISSN: 1365-2966
PURE UUID: e75db383-429d-4774-a6d9-df9a1b4ae19a
ORCID for D. Altamirano: ORCID iD orcid.org/0000-0002-3422-0074
ORCID for P. Gandhi: ORCID iD orcid.org/0000-0003-3105-2615

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Date deposited: 17 Nov 2025 17:59
Last modified: 18 Nov 2025 02:47

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Contributors

Author: A.K. Hughes
Author: F. Carotenuto
Author: T.D. Russell
Author: A.J. Tetarenko
Author: J.C.A. Miller-Jones
Author: R.M. Plotkin
Author: A. Bahramian
Author: J.S. Bright
Author: F.J. Cowie
Author: J. Crook-Mansour
Author: R. Fender
Author: J.K. Khaulsay
Author: A. Kirby
Author: S. Jones
Author: M. McCollough
Author: R. Rao
Author: G.R. Sivakoff
Author: S.D. Vrtilek
Author: D.R.A. Williams-Baldwin
Author: C.M. Wood
Author: D. Altamirano ORCID iD
Author: P. Casella
Author: N. Castro Segura
Author: S. Corbel
Author: M. Del Santo
Author: C. Echiburu-Trujillo
Author: J. van den Eijnden
Author: E. Gallo
Author: P. Gandhi ORCID iD
Author: K.I.I. Koljonen
Author: T. Maccarone
Author: S.B. Markoff
Author: S. Motta
Author: D.M. Russell
Author: P. Saikia
Author: A.W. Shaw
Author: R. Soria
Author: J.A. Tomsick
Author: W. Yu
Author: X. Zhang
Corporate Author: et al.

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