The 2020 superburst of 4U 1608–522 and its impact on the accretion disc

ABSTRACT Superbursts are rare events observed from bursting neutron star low-mass X-ray binaries. They are thought to originate from unstable burning of the thick layer of Carbon on the surface of the neutron star, causing the observed X-ray flashes to last several hours. Given their fluence it has long been thought that superbursts may have significant effects on the accretion flow around the neutron star. In this paper, we first present evidence for a new superburst observed from 4U 1608–522 by Monitor of All-sky X-ray Image (MAXI) during the 2020 outburst, around 00:45 utc on 2020 July 16. We compare some of the properties of this superburst and the underlying outburst with the events recorded on 2005 May 5 by Rossi X-ray Timing Explorer (RXTE) and most recently in 2025 by MAXI. We then present our spectral analysis of Neutron star Interior Composition Explorer (NICER) and Insight–HXMT data obtained before and after the 2020 superburst event. Our results indicate that the inner disc temperature and the radius show a systematic evolution in the following few days, which may be related to the superburst. We show that the time-scale of the observed evolution can not be governed by viscous time-scales unless the viscosity parameter is unrealistically low.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-09-09
DOI
https://doi.org/10.1093/mnras/staf1502
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.00

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article

The 2020 superburst of 4U 1608–522 and its impact on the accretion disc

Tuğba Boztepe, Gaurava K. Jaisawal, A. Sanna, Elif Ece Devecioğlu et al.
Monthly Notices of the Royal Astronomical Society
Astrophysical Phenomena and Observations
article

The 2020 superburst of 4U 1608–522 and its impact on the accretion disc

Tuğba Boztepe, Gaurava K. Jaisawal, A. Sanna, Elif Ece Devecioğlu, W. Iwakiri, Can Güngör, D. Altamirano, Mason Ng, D. R. Ballantyne, J. Speicher, Tolga Güver, Motoko Serino
article en

Abstract

ABSTRACT Superbursts are rare events observed from bursting neutron star low-mass X-ray binaries. They are thought to originate from unstable burning of the thick layer of Carbon on the surface of the neutron star, causing the observed X-ray flashes to last several hours. Given their fluence it has long been thought that superbursts may have significant effects on the accretion flow around the neutron star. In this paper, we first present evidence for a new superburst observed from 4U 1608–522 by Monitor of All-sky X-ray Image (MAXI) during the 2020 outburst, around 00:45 utc on 2020 July 16. We compare some of the properties of this superburst and the underlying outburst with the events recorded on 2005 May 5 by Rossi X-ray Timing Explorer (RXTE) and most recently in 2025 by MAXI. We then present our spectral analysis of Neutron star Interior Composition Explorer (NICER) and Insight–HXMT data obtained before and after the 2020 superburst event. Our results indicate that the inner disc temperature and the radius show a systematic evolution in the following few days, which may be related to the superburst. We show that the time-scale of the observed evolution can not be governed by viscous time-scales unless the viscosity parameter is unrealistically low.

Monthly Notices of the Royal Astronomical SocietyVol. 543(2)
Space Science Institute (US), Georgia Institute of Technology (US), Aoyama Gakuin University (JP), Chiba University (JP), State Street (United States) (US), Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari (IT), Astronomy and Space (AU), University of Southampton (GB), McGill University (CA), Istanbul University (TR), Technical University of Denmark (DK)
National Aeronautics and Space Administration, Georgia Institute of Technology, Goddard Space Flight Center, Fonds de recherche du Québec – Nature et technologies, Japan Aerospace Exploration Agency, RIKEN, Astrophysics Science Division
Openalex Percentile: Top 83%
Astrophysical Phenomena and Observations
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