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Related papers: Transient X-ray pulsar V0332+53: pulse phase-resol…

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We report on optical and RXTE observations of a new high-latitude bursting X-ray transient, XTE J2123-058. We identified the optical counterpart, measured the 5.9573 hr orbital period and constrained the binary inclination and the source…

Astrophysics · Physics 2009-10-31 John A. Tomsick , Jules P. Halpern , Jonathan Kemp , Philip Kaaret

We report on an XMM-Newton observation of the accreting millisecond pulsar, IGR J17511-3057. Pulsations at 244.8339512(1) Hz are observed with an RMS pulsed fraction of 14.4(3)%. A precise solution for the P_orb=12487.51(2)s binary system…

High Energy Astrophysical Phenomena · Physics 2015-05-19 A. Papitto , A. Riggio , T. Di Salvo , L. Burderi , A. D'Aì , R. Iaria , E. Bozzo , M. T. Menna

The Rossi X-ray Timing Explorer ({\sl RXTE}) has made hundreds of observations on three famous young pulsars (PSRs) B0531+21 (Crab), B1509-58, and B0540-69. Using the archive {\sl RXTE} data, we have studied the phase-resolved spectral…

High Energy Astrophysical Phenomena · Physics 2012-04-11 M. Y. Ge , F. J. Lu , J. L. Qu , S. J. Zheng , Y. Chen , D. W. Han

Three observations of the 5.54 s Transient Anomalous X-ray Pulsar XTE J1810-197 obtained over 6 months with the Newton X-Ray Multi-Mirror Mission (XMM-Newton) are used to study its spectrum and pulsed light curve as the source fades from…

Astrophysics · Physics 2009-11-10 J. P. Halpern , E. V. Gotthelf

We present the results of observations of XTE J0421+560 X-ray transient with Rossi X-ray Timing Explorer in the beginning of April 1998. Lightcurve, obtained by ASM all-sky monitor, shows unusually fast decrease in the object's luminosity.…

Astrophysics · Physics 2007-05-23 M. Revnivtsev , A. Emelyanov , K. Borozdin

A0535+262 is a transient Be/X-ray binary system which was in a quiescent phase from 1994-2005. In this paper we report on the timing and spectral properties of the INTEGRAL detection of the source in October 2003. The source is detected for…

A bright X-ray transient was seen during an XMM-Newton observation in the direction of the Small Magellanic Cloud (SMC) in October 2006. The EPIC data allow us to accurately locate the source and to investigate its temporal and spectral…

Astrophysics · Physics 2009-11-13 F. Haberl , W. Pietsch

We model the pulse profiles and the phase resolved spectra of the anomalous X-ray pulsar 1E 1048.1-5937 obtained with XMM-Newton to map its surface temperature distribution during an active and a quiescent epoch. We develop and apply a…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Tolga Guver , Ersin Gogus , Feryal Ozel

The X-ray source 4U 1822-371 is an eclipsing low-mass X-ray binary and X-ray pulsar, hosting a NS that shows periodic pulsations in the X-ray band. The inclination angle of the system is so high that in principle, it should be hard to…

High Energy Astrophysical Phenomena · Physics 2021-10-27 A. Anitra , T. Di Salvo , R. Iaria , L. Burderi , A. F. Gambino , S. M. Mazzola , A. Marino , A. Sanna , A. Riggio

Aims: We investigate the X-ray spectral and timing properties of the accreting X-ray pulsar Her X-1 observed with the INTEGRAL satellite in July-August 2005. Methods: The data analyzed in this work cover a substantial part of one main-on…

We present the first detailed joint modelling of both the timing and spectral properties during the outburst decay of transient anomalous X-ray pulsars. We consider the two sources XTE J1810-197 and CXOU J164710.2-455216, and describe the…

High Energy Astrophysical Phenomena · Physics 2015-05-27 S. Zane , A. Albano , R. Turolla , G. L. Israel , L. Nobili , L. Stella

The X-ray binary pulsar Her X-1 shows a wide variety of long and short term variabilities in the X-ray light curve. The 35 d variability of the source is interpreted as the influence of a warped, inclined, and twisted accretion disk…

Astrophysics · Physics 2007-05-23 M. Kuster , J. Wilms , R. Staubert , P. Risse , W. A. Heindl , R. Rothschild , N. I. Shakura , K. A. Postnov

The well known black-hole X-ray binary transient XTE J1550-564 underwent an outburst during the spring of 2003 which was substantially underluminous in comparison to previous periods of peak activity in that source. In addition, our…

Astrophysics · Physics 2009-11-10 S. J. Sturner , C. R. Shrader

We report the timing and broad-band spectral properties of the Be transient high mass X-ray binary pulsar GRO J1008-57 using a Suzaku observation in the declining phase of its 2007 November-December outburst. Pulsations with a period of…

Solar and Stellar Astrophysics · Physics 2011-05-17 Sachindra Naik , Biswajit Paul , Chetan Kachhara , Santosh V. Vadawale

We present high-speed optical photometry of the anomalous X-ray pulsar 1E 1048.1-5937 obtained with ULTRACAM on the 8.2-m Very Large Telescope in June 2007. We detect 1E 1048.1-5937 at a magnitude of i'=25.3+/-0.2, consistent with the…

High Energy Astrophysical Phenomena · Physics 2009-11-13 V. S. Dhillon , T. R. Marsh , S. P. Littlefair , C. M. Copperwheat , P. Kerry , R. Dib , M. Durant , V. M. Kaspi , R. P. Mignani , A. Shearer

We have monitored a Type II outburst of the Be/X-ray binary MXB 0656-072 in a series of pointed RXTE observations during October through December 2003. The source spectrum shows a cyclotron resonance scattering feature at 32.8 +/- 0.5 keV,…

We report the results of a recent (July 2004) XMM-Newton Target of Opportunity observation of the Anomalous X-ray pulsar 1E 1048.1-5937, together with a detailed re-analysis of previous observations carried out in 2000 and 2003. In July…

Astrophysics · Physics 2009-11-10 A. Tiengo , S. Mereghetti , R. Turolla , S. Zane , N. Rea , L. Stella , G. L. Israel

We present a first INTEGRAL observation of the 42s transient X-ray pulsar EXO 2030+375 with IBIS/ISGRI. The source was detected during Cyg X-1 observations in December 2002. We analyzed observations during the outburst period from 9 to 21…

We analyze the properties of the pulsed emission from the accreting millisecond pulsar SAX J1808.4-3658 in observations of its April 1998 outburst by the Rossi X-Ray Timing Explorer. Pulse phase spectroscopy shows that the emission evolves…

Astrophysics · Physics 2009-10-31 Eric C. Ford

We present NICER observations of accreting X-ray pulsar 1A 0535+262 during its faint state ($\lesssim 6\times10^{36}$ erg/s) observed in several type I and II outbursts. We discovered a transition of temporal and spectral properties around…

High Energy Astrophysical Phenomena · Physics 2024-04-02 Hua Xiao , Long Ji