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Synchronous X-ray/optical quasi-periodic oscillations from the black hole LMXB MAXI J1820+070

Synchronous X-ray/optical quasi-periodic oscillations from the black hole LMXB MAXI J1820+070
Synchronous X-ray/optical quasi-periodic oscillations from the black hole LMXB MAXI J1820+070
We present high-speed optical photometry from SAAO and SALT on the black hole LMXB MAXI J1820+070 (ASSASN-18ey), some of it simultaneous with NICER, Swift, and Insight-HXMT X-ray coverage. We detect optical quasi-periodic oscillations (QPOs) that move to higher frequencies as the outburst progresses, tracking both the frequency and evolution of similar X-ray QPOs previously reported. Correlated X-ray/optical data reveal a complex pattern of lags, including an anticorrelation and a sub-second lag that evolve over the first few weeks of outburst. They also show correlated components separated by a lag equal to the QPO period roughly centered on zero lag, implying that the inter-band variability is strongly and consistently affected by these QPOs at a constant phase lag of roughly ±π. The synchronization of X-ray and optical QPOs indicates that they must be produced in regions physically very close to each other; we, thus, propose that they can be explained by a precessing jet model, based on analogies with V404 Cyg and MAXI J1348-630.
accretion, accretion discs, black hole physics, stars: individual: MAXI J1820+070
1745-3925
Thomas, Jessymol K.
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Buckley, David A. H.
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Charles, Philip A.
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Paice, John A.
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Potter, Stephen B.
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Steiner, James F.
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Lasota, Jean-Pierre
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Gandhi, P.
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Tao, Lian
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Ma, Xiang
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Yang, Yi-Jung
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Tuo, Youli
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Zhang, Shuang-Nan
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et al.
Thomas, Jessymol K.
a7f79e38-fc16-4a77-93e8-52d948aa839d
Buckley, David A. H.
219e118a-8a7d-4a68-826c-3df498795832
Charles, Philip A.
0429b380-0754-4dc1-8def-885c7fa6a086
Paice, John A.
8ac21dae-fc44-4797-b2aa-31125c9172ae
Potter, Stephen B.
2a96dd31-566f-4a66-b888-67860ece7fa5
Steiner, James F.
7f446296-425e-4236-9ea7-a7d2694a90b5
Lasota, Jean-Pierre
0eb03a33-d77c-489d-b402-47b9c95a0eec
Gandhi, P.
5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
Tao, Lian
75749bbb-a4e9-4734-8325-6180e5dad82b
Ma, Xiang
e00054e2-db8d-44c6-be6c-7cf807f0f6d3
Yang, Yi-Jung
63adefda-516a-4bd3-820d-07f645e07635
Tuo, Youli
114d696b-7754-468a-b6ba-db3ee9102c81
Zhang, Shuang-Nan
3cb9d0a2-8546-43d8-a94c-2b5816c42bd3

Thomas, Jessymol K., Buckley, David A. H., Charles, Philip A., Paice, John A. and Gandhi, P. , et al. (2022) Synchronous X-ray/optical quasi-periodic oscillations from the black hole LMXB MAXI J1820+070. Monthly Notices of the Royal Astronomical Society: Letters, 513 (1). (doi:10.1093/mnrasl/slab132).

Record type: Article

Abstract

We present high-speed optical photometry from SAAO and SALT on the black hole LMXB MAXI J1820+070 (ASSASN-18ey), some of it simultaneous with NICER, Swift, and Insight-HXMT X-ray coverage. We detect optical quasi-periodic oscillations (QPOs) that move to higher frequencies as the outburst progresses, tracking both the frequency and evolution of similar X-ray QPOs previously reported. Correlated X-ray/optical data reveal a complex pattern of lags, including an anticorrelation and a sub-second lag that evolve over the first few weeks of outburst. They also show correlated components separated by a lag equal to the QPO period roughly centered on zero lag, implying that the inter-band variability is strongly and consistently affected by these QPOs at a constant phase lag of roughly ±π. The synchronization of X-ray and optical QPOs indicates that they must be produced in regions physically very close to each other; we, thus, propose that they can be explained by a precessing jet model, based on analogies with V404 Cyg and MAXI J1348-630.

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Accepted/In Press date: 24 December 2021
Published date: 1 June 2022
Keywords: accretion, accretion discs, black hole physics, stars: individual: MAXI J1820+070

Identifiers

Local EPrints ID: 475633
URI: http://eprints.soton.ac.uk/id/eprint/475633
ISSN: 1745-3925
PURE UUID: 641f86b0-bd38-477e-b608-4276af658cd9
ORCID for P. Gandhi: ORCID iD orcid.org/0000-0003-3105-2615

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Date deposited: 23 Mar 2023 17:31
Last modified: 17 Mar 2024 03:37

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Contributors

Author: Jessymol K. Thomas
Author: David A. H. Buckley
Author: John A. Paice
Author: Stephen B. Potter
Author: James F. Steiner
Author: Jean-Pierre Lasota
Author: P. Gandhi ORCID iD
Author: Lian Tao
Author: Xiang Ma
Author: Yi-Jung Yang
Author: Youli Tuo
Author: Shuang-Nan Zhang
Corporate Author: et al.

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