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相关论文: NuSTAR view of Be/X-ray binary pulsar 2S 1417-624 …

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We present the results obtained from timing and spectral studies of the accretion powered X-ray pulsar 2S~1417-624 during a giant outburst in 2009 by using {\it Rossi X-ray Timing Explorer (RXTE)} observations. X-ray pulsations were…

高能天体物理现象 · 物理学 2018-07-25 Shivangi Gupta , Sachindra Naik , Gaurava K. Jaisawal , Prahlad R. Epili

We report results from a multi-mission observational campaign of the transient X-ray pulsar 2S~1417$-$624 during its 2025 outburst, using data from NICER, IXPE, and NuSTAR. Phase-averaged and phase-resolved spectroscopy with NICER and…

We study the timing and spectral properties of the X-ray pulsar 2S 1417--624 during the recent outburst in January 2021 based on the Neutron Star Interior Composition Explorer (NICER) observation. We also used some early data from the 2018…

高能天体物理现象 · 物理学 2022-11-28 Manoj Mandal , Sabyasachi Pal

The Be X-ray binary GRO J2058+42 recently went through a Type-II outburst during March-April 2019 lasting for about 50 days. This outburst was detected with the operating all sky X-ray monitors like the Fermi-GBM, Swift-BAT and MAXI-GSC.…

高能天体物理现象 · 物理学 2020-07-22 Sanhita Kabiraj , Biswajit Paul

The Be X-ray pulsar (BeXRP) SXP 59 underwent a giant outburst in 2017 with a peak X-ray luminosity of $1.1\times10^{38}$ erg~s$^{-1}$. We report on the X-ray behaviour of SXP 59 with the XMM--Newton and NuSTAR observations collected at the…

高能天体物理现象 · 物理学 2019-09-19 Shan-Shan Weng , Ming-Yu Ge , Hai-Hui Zhao

We report comprehensive spectral and temporal properties of the Be/X-ray binary pulsar SMC X-2 using X-ray observations during the 2015 and 2022 outbursts. The pulse profile of the pulsar is unique and strongly luminosity dependent. It…

高能天体物理现象 · 物理学 2023-03-21 G. K. Jaisawal , G. Vasilopoulos , S. Naik , C. Maitra , C. Malacaria , B. Chhotaray , K. C. Gendreau , S. Guillot , M. Ng , A. Sanna

We present results of detailed investigation of the poorly studied X-ray pulsar 2S 1845$-$024 based on the data obtained with $NuSTAR$ observatory during the type I outburst in 2017. Neither pulse phase-averaged, nor phase-resolved spectra…

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 a detailed timing and spectral analysis of the X-ray pulsar 2S~1417-624 using the data from Insight-HXMT during the 2018 outburst. The pulse profiles are highly variable with respect to both unabsorbed flux and energy. A…

高能天体物理现象 · 物理学 2024-10-31 Q. Liu , A. Santangelo , L. D. Kong , L. Ducci , L. Ji , W. Wang , M. M. Serim , C. Güngör , Y. L. Tuo , D. Serim

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

The Be X-ray pulsar SMC X-3 underwent an extra long and ultraluminous giant outburst from 2016 August to 2017 March. The peak X-ray luminosity is up to $\sim 10^{39}$ erg/s, suggesting a mildly super-Eddington accretion onto the strongly…

高能天体物理现象 · 物理学 2018-01-17 Hai-Hui Zhao , Shan-Shan Weng , Ming-Yu Ge , Wei-Hao Bian , Qi-Rong Yuan

We present an extended study of the Be/X-ray pulsar 2S 1553-542 during its Type II outbursts. We have incorporated \emph{NICER, Swift-XRT, RXTE-PCA, \emph{NuSTAR} and FERMI} observations to carry out the detailed phase and time resolved…

高能天体物理现象 · 物理学 2023-05-10 Binay Rai , Biswajit Paul , Mohammed Tobrej , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We present the results obtained from the analysis of high mass X-ray binary pulsar 4U 1909+07 using NuSTAR and Astrosat observations in 2015 and 2017 July, respectively. X-ray pulsations at $\approx$604 s are clearly detected in our study.…

高能天体物理现象 · 物理学 2020-08-26 Gaurava K. Jaisawal , Sachindra Naik , Wynn C. G. Ho , Neeraj Kumari , Prahlad Epili , Georgios Vasilopoulos

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

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 present a detailed spectro-temporal study of the Be X-ray binary pulsar $1A$ $1118-61$ during its brightest recorded outburst in 2026, using \textit{Swift} and \textit{NuSTAR} observations, and compare its properties with the 2009…

高能天体物理现象 · 物理学 2026-05-19 Kinjal Roy , Aru Beri , Rahul Sharma , Phil Charles

We report results of a spectral and timing analysis of the poorly studied transient X-ray pulsar 2S 1553-542 using data collected with the NuSTAR and Chandra observatories and the Fermi/GBM instrument during an outburst in 2015. Properties…

We present a spectral study of the ultraluminous Be/X-ray transient pulsar Swift J0243.6+6124 using Neutron Star Interior Composition Explorer (NICER) observations during the system's 2017--2018 giant outburst. The 1.2--10~keV energy…

We study the timing and spectral properties of the X-ray pulsar 2S 1553--542 using the NuSTAR, and NICER during the outburst in January--February 2021. During the outburst, the spin period of the neutron star was 9.2822 s based on NuSTAR…

星系天体物理 · 物理学 2023-06-22 Manoj Mandal , Sabyasachi Pal

We investigate timing and spectral characteristics of the transient X-ray pulsar 2S 1417$-$624 during its 2018 outburst with \emph{NICER} follow up observations. We describe the spectra with high-energy cut-off and partial covering fraction…

高能天体物理现象 · 物理学 2021-12-15 M. M. Serim , O. C. Ozudogru , C. K. Donmez , S. Sahiner , D. Serim , A. Baykal , S. C. Inam
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