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We have monitored the transient neutron star low-mass X-ray binary 1RXS J180408.9-342058 in quiescence after its ~4.5 month outburst in 2015. The source has been observed using Swift and XMM-Newton. Its X-ray spectra were dominated by a…

We model the spectral formation occurring in the binary X-ray pulsar RX~J0209.6-7427 during the 2019 super-Eddington outburst. Using a theoretical model previously developed by the authors, we are able to produce spectra that closely…

High Energy Astrophysical Phenomena · Physics 2024-04-26 Brent F. West , Peter A. Becker , Georgios Vasilopoulos

Superbursts from accreting neutron stars probe nuclear reactions at extreme densities ($\rho \approx 10^{9}~g\,cm^{-3}$) and temperatures ($T>10^9~K$). These bursts ($\sim$1000 times more energetic than type I X-ray bursts) are most likely…

Solar and Stellar Astrophysics · Physics 2015-06-19 Jeremy Stevens , Edward F. Brown , Andrew Cumming , Richard Cyburt , Hendrik Schatz

We present the results obtained from timing and spectral studies of 15 thermonuclear X-ray bursts from 4U 1820-30 observed with the Neutron Star Interior Composition Explorer (NICER) during its five years of observations between 2017-2022.…

We study 15 thermonuclear X-ray bursts from 4U 1820--30 observed with the Neutron Star Interior Composition Explorer (NICER). We find evidence of a narrow emission line at 1.0 keV and three absorption lines at 1.7, 3.0, and 3.75 keV,…

On 28 February 2007 a new outburst of the previously known transient source XTE J1856+053 was detected with RXTE/ASM. We present here the results of an XMM-Newton (0.5-10.0 keV) Target of Opportunity observation performed on 14 March 2007,…

Astrophysics · Physics 2011-08-31 G. Sala , J. Greiner , M. Ajello , N. Primak

We report the temporal and spectral analysis of three thermonuclear X-ray bursts from 4U 1608-52, observed by the Neutron Star Interior Composition Explorer (NICER) during and just after the outburst observed from the source in 2020. In two…

Neutron stars accreting matter from low-mass binary companions are observed to undergo bursts of X-rays due to the thermonuclear explosion of material on the neutron star surface. We use recent results on superfluid and superconducting…

High Energy Astrophysical Phenomena · Physics 2012-01-17 Wynn C. G. Ho

We report the detection of a long X-ray burst triggered on MJD 60171.65 from the ultra-compact binary 4U 1850$-$087 by the Monitor of All-sky X-ray Image and Neutron Star Interior Composition Explorer (NICER). We analyse the NICER data…

High Energy Astrophysical Phenomena · Physics 2024-07-31 Yongqi Lu , Zhaosheng Li , Wenhui Yu , Yuanyue Pan , Maurizio Falanga

We investigate the X-ray spectrum, variability and the surrounding ionized bubble of NGC1313 X-2 to explore the physics of super-Eddington accretion. Beyond the Eddington luminosity, the accretion disk of NGC1313 X-2 is truncated at a large…

High Energy Astrophysical Phenomena · Physics 2015-11-25 Shan-Shan Weng , Shuang-Nan Zhang , Hai-Hui Zhao

Rare, energetic (long) thermonuclear (Type I) X-ray bursts are classified either as intermediate-duration or superbursts, based on their duration. Intermediate-duration bursts lasting a few to tens of minutes are thought to arise from the…

We consider fallback accretion after an ultra-stripped supernova (USSN) that accompanies formation of a binary neutron star (BNS) or a neutron star-black hole binary (NS-BH). The fallback matter initially accretes directly to the nascent…

High Energy Astrophysical Phenomena · Physics 2022-08-31 Kazumi Kashiyama , Ryo Sawada , Yudai Suwa

A comprehensive wideband spectral analysis of the brightest black hole X-ray binary 4U $1543-47$ during its 2021 outburst is carried out for the first time using NICER, NuSTAR, and AstroSat observations by phenomenological and reflection…

High Energy Astrophysical Phenomena · Physics 2023-02-02 Geethu Prabhakar , Samir Mandal , Bhuvana G. R. , Anuj Nandi

(abridged version) We report on ten type I X-ray bursts from GX 17+2 in data obtained with the RXTE/PCA in 1996--2000. Three bursts were short in duration (~10 s), whereas the others lasted for ~6-25 min. Five of the long bursts showed…

Astrophysics · Physics 2009-11-06 E. Kuulkers , J. Homan , M. van der Klis , W. H. G. Lewin , M. Mendez

We report on the results obtained by the analysis of persistent and type-I thermonuclear X-ray burst emission observed from the periodic burster 4U 1323-62. These analyses are based on the NuSTAR observation performed on 2024 August 7 for a…

High Energy Astrophysical Phenomena · Physics 2026-01-06 Mahasweta Bhattacharya , Aditya S. Mondal , Biplab Raychaudhuri , Gulab C. Dewangan

Type-I X-ray bursts observed from neutron stars originate from intermittent unstable thermonuclear burning of accreted matter on these stars. Such bursts, particularly those reaching the Eddington luminosity and having a temporary…

High Energy Astrophysical Phenomena · Physics 2025-09-03 Sudip Bhattacharyya , Akshay Singh , Andrea Sanna

We perform a comprehensive study of thermonuclear bursts from the neutron star low-mass X-ray binary 4U 1702-429 detected with NICER and XMM-Newton. The thermonuclear burst detected with NICER shows clear evidence of a photospheric radius…

High Energy Astrophysical Phenomena · Physics 2025-08-19 Manoj Mandal , Sachindra Naik , Gaurava Kumar Jaisawal

We report on two new quiescent {\it XMM-Newton} observations (in addition to the earlier {\it Swift}/XRT and {\it XMM-Newton} coverage) of the cooling neutron star crust in the low-mass X-ray binary 1RXS J180408.9$-$342058. Its crust was…

High Energy Astrophysical Phenomena · Physics 2018-03-14 A. S. Parikh , R. Wijnands , N. Degenaar , L. Ootes , D. Page

We analysed Rossi X-ray Timing Explorer observations of the accretion-powered 401 Hz pulsar SAX J1808.4-3658, in order to precisely determine the source distance. While the fluences for the five transient outbursts observed from 1996 were…

Astrophysics · Physics 2011-02-11 Duncan Galloway , Andrew Cumming

On 2025 January 10, a thermonuclear (Type I) X-ray burst from the neutron star low-mass X-ray binary \textit{4U~0614+091} was detected with the ECLAIRs instrument on board the \textit{SVOM} mission. We present here a time-resolved…

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