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相关论文: Timing and spectral analysis of 2S 1417$-$624 duri…

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We report on the phase-coherent timing analysis of the accreting millisecond X-ray pulsar IGR J17591-2342, using Neutron Star Interior Composition Explorer (NICER) data taken during the outburst of the source between 2018 August 15 and 2018…

高能天体物理现象 · 物理学 2020-05-13 A. Sanna , L. Burderi , K. C. Gendreau , T. Di Salvo , P. S. Ray , A. Riggio , A. F. Gambino , R. Iaria , L. Piga , C. Malacaria , G. K. Jaisawal

We discuss the spectral and timing properties of the accreting millisecond X-ray pulsar SWIFT J1756.9-2508 observed by XMM-Newton, NICER and NuSTAR during the X-ray outburst occurred in April 2018. The spectral properties of the source are…

高能天体物理现象 · 物理学 2018-09-05 A. Sanna , F. Pintore , A. Riggio , S. M. Mazzola , E. Bozzo , T. Di Salvo , C. Ferrigno , A. F. Gambino , A. Papitto , R. Iaria , L. Burderi

The Be/X-ray binary 1A 0535+262 underwent a giant X-ray outburst in November 2020, peaking at $\sim1\times 10^{38}$ erg s$^{-1}$ (1--100 keV, 1.8 kpc), the brightest outburst recorded for this source so far. Our goal is to search for…

高能天体物理现象 · 物理学 2022-03-30 P. Reig , R. C. Ma , L. Tao , S. Zhang , S. N. Zhang , V. Doroshenko

In this paper we present a coherent timing analysis of the 401 Hz pulsations of the accreting millisecond X-ray pulsar SAX J1808.4-3658 during its 2019 outburst. Using observations collected with the Neutron Star Interior Composition…

We present the results obtained from timing and spectral studies of the newly discovered accreting X-ray binary pulsar Swift J0243.6+6124 using a NuSTAR observation in 2017 October at a flux level of ~280 mCrab. Pulsations at 9.85423(5) s…

高能天体物理现象 · 物理学 2017-11-30 Gaurava K. Jaisawal , Sachindra Naik , J. Chenevez

We report on X-ray and radio observations of the ultra-compact X-ray binary 4U 1543-624 taken in August 2017 during an enhanced accretion episode. We obtained NICER monitoring of the source over a $\sim10$ day period during which…

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…

高能天体物理现象 · 物理学 2024-04-26 Brent F. West , Peter A. Becker , Georgios Vasilopoulos

The Rossi X-ray Timing Explorer has observed five outbursts from the transient 2.5 ms accretion-powered pulsar SAX J1808.4-3658 during 1998-2008. We present a pulse timing study of the most recent outburst and compare it with the previous…

高能天体物理现象 · 物理学 2009-09-28 J. M. Hartman , A. Patruno , D. Chakrabarty , C. B. Markwardt , E. H. Morgan , M. van der Klis , R. Wijnands

This work presents the first ever broadband (0.7-25.0 keV) timing and spectral analysis of Be-HMXB 2S 1417-624 during its 2021 outburst. Using AstroSat observations, coherent pulsations at ~17.36633 s (MJD 59239.082) were detected in…

高能天体物理现象 · 物理学 2024-07-30 Chetana Jain

We report on our investigation of the NuSTAR and AstroSat observations along with simultaneous NICER observations of the accreting millisecond X-ray pulsar SAX J1808.4$-$3658, obtained during its tenth outburst from 2022. The NuSTAR…

高能天体物理现象 · 物理学 2026-02-16 Rahul Sharma , Andrea Sanna , Prince Sharma

We present a 7 yr timing study of the 2.5 ms X-ray pulsar SAX J1808.4-3658, an X-ray transient with a recurrence time of ~2 yr, using data from the Rossi X-ray Timing Explorer covering 4 transient outbursts (1998-2005). We verify that the…

The November 1999 outburst of the transient pulsar SAX J2103.5+4545 was monitored with the large area detectors of the Rossi X-Ray Timing Explorer until the pulsar faded after a year. The 358 s pulsar was spun up for 150 days, at which…

天体物理学 · 物理学 2009-11-07 A. Baykal , M. J. Stark , J. H. Swank

We present timing and spectral results of 2018 outburst of Cepheus X-4, observed twice by AstroSat at luminosity of $2.04 \times 10^{37}$ erg s$^{-1}$ and $1.02 \times 10^{37}$ erg s$^{-1}$ respectively. The light curves showed strong…

高能天体物理现象 · 物理学 2021-11-03 Kallol Mukerjee , H. M. Antia

In the beginning of 2023 the Be transient X-ray pulsar RX J0440.9+4431 underwent a fist-ever giant outburst observed from the source peaking in the beginning of February and reaching peak luminosity of $\sim 4.3\times10^{37}$ erg s$^{-1}$.…

We conduct a detailed spectral analysis of the Galactic ultraluminous X-ray pulsar Swift J0243.6+6124 in its sub-Eddington regime, using Insight-HXMT and NICER observations during multiple outbursts including the 2018 giant outburst. We…

The Neutron Star X-ray binary Sco X-1 is one of the brightest Z-type sources in our Galaxy, showing frequent periods of flaring activity and different types of relativistic outflows. Observations with RXTE have shown that the strongest…

高能天体物理现象 · 物理学 2025-09-17 J. López-Miralles , S. E. Motta , J. C. A. Miller-Jones , J. Homan , J. Kajava , S. Migliari

We report the results provided by the XMM-Newton observation of the X-ray binary pulsar SXP59.0 during its most recent outburst in April 2017. The source was detected at $f_{\rm X}$(0.2-12 keV) = 8$\times 10^{-11}$ erg cm$^{-2}$ s$^{-1}$,…

高能天体物理现象 · 物理学 2018-11-21 N. La Palombara , P. Esposito , F. Pintore , L. Sidoli , S. Mereghetti , A. Tiengo

We made a detailed study of the timing and spectral properties of the X-ray pulsar 1A 0535+262 during the recent giant outburst in 2020 November and December. The flux of the pulsar reached a record value of $\sim$12.5 Crab as observed by…

高能天体物理现象 · 物理学 2022-03-11 Manoj Mandal , Sabyasachi Pal

We present a pulse timing analysis of NICER observations of the accreting millisecond X-ray pulsar SAX J1808.4$-$3658 during the outburst that started on 2022 August 19. Similar to previous outbursts, after decaying from a peak luminosity…

We present the spectral and timing evolution of the persistent black hole X-ray binary GRS 1758-258 based on almost 12 years of observations using the Rossi X-ray Timing Explorer Proportional Counter Array. While the source was…