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相关论文: 4U 1626-67 Returns to Spin-Down: Timing features t…

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We report the discovery with the Proportional Counter Array on board the Rossi X-ray Timing Explorer of highly coherent 582 Hz pulsations during the February 22, 2001 (UT) ``superburst'' from 4U 1636-53. The pulsations are detected during…

天体物理学 · 物理学 2008-11-26 Tod E. Strohmayer , Craig. B. Markwardt

On 2011 July 14, a new magnetar candidate, Swift J1822.3-1606, was identified via a rate trigger on the Swift/Burst Alert Telescope. Here we present an initial analysis of the X-ray properties of the source, using data from the Rossi X-ray…

高能天体物理现象 · 物理学 2015-05-30 Margaret A. Livingstone , Paul Scholz , Victoria M. Kaspi , C. -Y. Ng , Fotis P. Gavriil

We present the timing and spectral analysis of the HMXB source 4U 1538-522 using NuSTAR observations. One of the observations partially covers the X-ray eclipse of the source along with eclipse ingress. The source is found to spin down at…

高能天体物理现象 · 物理学 2023-10-02 Ruchi Tamang , Manoj Ghising , Mohammed Tobrej , Binay Rai , Bikash Chandra Paul

We report timing and spectral studies of the high mass X-ray binary 4U 1700-37 using Insight-HXMT observations carried out in 2020 during its out-of-eclipse state. We found significant variations in flux on a time-scale of kilo-seconds,…

高能天体物理现象 · 物理学 2024-04-02 Hua Xiao , Long Ji , Peng Zhang , Lorenzo Ducci , Victor Doroshenko , Andrea Santangelo , Shu Zhang , Shuang-Nan Zhang

4U 0142+61 is one of a small class of persistently bright magnetars. Here we report on a monitoring campaign of 4U 0142+61 from 2011 July 26 - 2016 June 12 using the Swift X-ray Telescope, continuing a 16 year timing campaign with the Rossi…

高能天体物理现象 · 物理学 2017-01-18 R. F. Archibald , V. M. Kaspi , P. Scholz , A. P. Beardmore , N. Gehrels , J. A. Kennea

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

We analyze all X-ray timing data on 1E 1207.4-5209 in supernova remnant PKS 1209-51/52 gathered in 2000-2005, and find a highly stable rotation with P=424.130451(4) ms and period derivative of (9.6 +/- 9.4)E-17 s/s. This refutes previous…

天体物理学 · 物理学 2009-11-13 E. V. Gotthelf , J. P. Halpern

We present new observations of two anomalous X-ray pulsars (AXP) 4U 0142+61 and 1E 1048.1-5937 made in 1998 with the ASCA. The energy spectra of these two AXPs are found to consist of two components, a power-law and a blackbody emission…

天体物理学 · 物理学 2009-10-31 B. Paul , M. Kawasaki , T. Dotani , F. Nagase

X-ray observations of the accreting X-ray pulsar 4U~1907+09, obtained during February 1996 with the Proportional Counter Array on the Rossi X-ray Timing Experiment (RXTE), have enabled the first measurement of the intrinsic pulse period…

天体物理学 · 物理学 2009-10-30 J. J. M. in 't Zand , A. Baykal , T. E. Strohmayer

X-ray timing studies of the persistent, Galactic, accretion-powered pulsar 4U 1626$-$67 reveal torque reversals, during which the pulse frequency $\nu(t)$ alternates between multiyear episodes of secular acceleration and deceleration,…

Using Chandra data taken on 2008 June, we detected pulsations at 2.59439(4) s in the soft gamma-ray repeater SGR 1627-41. This is the second measurement of the source spin period and allows us to derive for the first time a long-term…

高能天体物理现象 · 物理学 2009-11-10 P. Esposito , M. Burgay , A. Possenti , R. Turolla , S. Zane , A. De Luca , A. Tiengo , G. L. Israel , F. Mattana , S. Mereghetti , M. Bailes , P. Romano , D. Götz , N. Rea

An overview of the results of observations for the transient X-ray pulsar 4U 0115+63, a member of a binary system with a Be star, since its discovery to the present day (~40 years) based on data from more than dozen observatories and…

高能天体物理现象 · 物理学 2015-06-16 P. A. Boldin , S. S. Tsygankov , A. A. Lutovinov

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

We present the broadband X-ray study of the BeXRB pulsar IGR J06074+2205 using NuSTAR observations. The temporal and spectral characteristics of the source are investigated. We detect coherent X-ray pulsations of the source and determine…

高能天体物理现象 · 物理学 2024-04-24 Mohammed Tobrej , Binay Rai , Manoj Ghising , Bikash Chandra Paul

The low-mass X-ray binary pulsar 4U 1626-67 shows 0.048 Hz quasi-periodic oscillations (QPOs) and red noise variability as well as coherent pulsations at the 0.130 Hz neutron star spin frequency. Power density spectra of observations made…

天体物理学 · 物理学 2009-10-30 J. M. Kommers , D. Chakrabarty , W. H. G. Lewin

We report on a timing and spectral analysis of a 50-ks NuSTAR observation of IGR J16320-4751 (= AX J1631.9-4752); a high-mass X-ray binary hosting a slowly-rotating neutron star. In this observation from 2015, the spin period was…

The NuSTAR hard X-ray telescope observed the transient Be/X-ray binary GS 0834-430 during its 2012 outburst - the first active state of this system observed in the past 19 years. We performed timing and spectral analysis, and measured the…

We report the results obtained from a detailed timing and spectral studies of Be/X-ray binary pulsar 2S 1417-624 using data from Swift and NuSTAR observatories. The observations were carried out at the peak of a giant outburst of the pulsar…

高能天体物理现象 · 物理学 2019-10-16 Shivangi Gupta , Sachindra Naik , Gaurava K. Jaisawal

In this paper we study the timing and spectral properties of Be/X-ray binary pulsar EXO 2030+375 using a $Suzaku$ observation on 2012 May 23, during a less intense Type I outburst. Pulsations were clearly detected in the X-ray light curves…

太阳与恒星天体物理 · 物理学 2015-06-23 Sachindra Naik , Gaurava K. Jaisawal

We report the results from a detailed timing and spectral study of transient X-ray pulsars, 4U 1901+03 during its 2019 outburst. We performed broadband spectroscopy in the 1-70 keV energy band using four observations made with Swift and…

高能天体物理现象 · 物理学 2020-11-04 Aru Beri , Tinku , Nirmal K. Iyer , Chandreyee Maitra