Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182

We report on the discovery of Swift J010902.6-723710, a rare eclipsing Be/X-ray Binary system by the Swift SMC Survey (S-CUBED). Swift J010902.6-723710 was discovered via weekly S-CUBED monitoring observations when it was observed to enter a state of X-ray outburst on 2023 October 10. X-ray emission...

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Main Authors: Thomas M. Gaudin, Jamie A. Kennea, M. J. Coe, I. M. Monageng, Andrzej Udalski, L. J. Townsend, David A. H. Buckley, Phil A. Evans
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/ad354a
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author Thomas M. Gaudin
Jamie A. Kennea
M. J. Coe
I. M. Monageng
Andrzej Udalski
L. J. Townsend
David A. H. Buckley
Phil A. Evans
author_facet Thomas M. Gaudin
Jamie A. Kennea
M. J. Coe
I. M. Monageng
Andrzej Udalski
L. J. Townsend
David A. H. Buckley
Phil A. Evans
author_sort Thomas M. Gaudin
collection DOAJ
description We report on the discovery of Swift J010902.6-723710, a rare eclipsing Be/X-ray Binary system by the Swift SMC Survey (S-CUBED). Swift J010902.6-723710 was discovered via weekly S-CUBED monitoring observations when it was observed to enter a state of X-ray outburst on 2023 October 10. X-ray emission was found to be modulated by a 182 s period. Optical spectroscopy is used to confirm the presence of a highly inclined circumstellar disk surrounding a B0-0.5Ve optical companion. Historical UV and IR photometry is then used to identify strong eclipse-like features reoccurring in both light curves with a 60.623 day period, which is adopted as the orbital period of the system. Eclipsing behavior is found to be the result of a large accretion disk surrounding the neutron star. Eclipses are produced when the disk passes in front of the OBe companion, blocking light from both the stellar surface and circumstellar disk. This is only the third Be/X-ray binary to have confirmed eclipses. We note that this rare behavior provides an important opportunity to constrain the physical parameters of a Be/X-ray binary with greater accuracy than is possible in noneclipsing systems.
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spelling doaj.art-4887c9becd79413dae573ebbad6197412024-04-05T10:35:03ZengIOP PublishingThe Astrophysical Journal Letters2041-82052024-01-019651L1010.3847/2041-8213/ad354aDiscovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182Thomas M. Gaudin0https://orcid.org/0009-0000-6957-8466Jamie A. Kennea1https://orcid.org/0000-0002-6745-4790M. J. Coe2https://orcid.org/0000-0002-0763-8547I. M. Monageng3https://orcid.org/0000-0002-4754-3526Andrzej Udalski4https://orcid.org/0000-0001-5207-5619L. J. Townsend5https://orcid.org/0000-0001-9788-3345David A. H. Buckley6https://orcid.org/0000-0002-7004-9956Phil A. Evans7https://orcid.org/0000-0002-8465-3353Pennsylvania State University , USAPennsylvania State University , USAPhysics and Astronomy, The University of Southampton , SO17 1BJ, UKSouth African Astronomical Observatory , PO Box 9, Observatory, Cape Town 7935, South Africa; Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701, South AfricaAstronomical Observatory, University of Warsaw , Al. Ujazdowskie 4, 00-478 Warszawa, PolandSouth African Astronomical Observatory , PO Box 9, Observatory, Cape Town 7935, South Africa; Southern African Large Telescope , PO Box 9, Observatory, Cape Town 7935, South AfricaSouth African Astronomical Observatory , PO Box 9, Observatory, Cape Town 7935, South Africa; Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701, South Africa; Southern African Large Telescope , PO Box 9, Observatory, Cape Town 7935, South Africa; Department of Astronomy, University of the Free State , PO Box 339, Bloemfontein, Cape Town 9300, South AfricaLeicester University , UKWe report on the discovery of Swift J010902.6-723710, a rare eclipsing Be/X-ray Binary system by the Swift SMC Survey (S-CUBED). Swift J010902.6-723710 was discovered via weekly S-CUBED monitoring observations when it was observed to enter a state of X-ray outburst on 2023 October 10. X-ray emission was found to be modulated by a 182 s period. Optical spectroscopy is used to confirm the presence of a highly inclined circumstellar disk surrounding a B0-0.5Ve optical companion. Historical UV and IR photometry is then used to identify strong eclipse-like features reoccurring in both light curves with a 60.623 day period, which is adopted as the orbital period of the system. Eclipsing behavior is found to be the result of a large accretion disk surrounding the neutron star. Eclipses are produced when the disk passes in front of the OBe companion, blocking light from both the stellar surface and circumstellar disk. This is only the third Be/X-ray binary to have confirmed eclipses. We note that this rare behavior provides an important opportunity to constrain the physical parameters of a Be/X-ray binary with greater accuracy than is possible in noneclipsing systems.https://doi.org/10.3847/2041-8213/ad354aHigh mass x-ray binary starsMassive starsX-ray binary starsHigh energy astrophysicsEclipsing binary stars
spellingShingle Thomas M. Gaudin
Jamie A. Kennea
M. J. Coe
I. M. Monageng
Andrzej Udalski
L. J. Townsend
David A. H. Buckley
Phil A. Evans
Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182
The Astrophysical Journal Letters
High mass x-ray binary stars
Massive stars
X-ray binary stars
High energy astrophysics
Eclipsing binary stars
title Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182
title_full Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182
title_fullStr Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182
title_full_unstemmed Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182
title_short Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182
title_sort discovery of a rare eclipsing be x ray binary system swift j010902 6 723710 sxp 182
topic High mass x-ray binary stars
Massive stars
X-ray binary stars
High energy astrophysics
Eclipsing binary stars
url https://doi.org/10.3847/2041-8213/ad354a
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