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

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The bright X-ray transient H 1743-322 was observed daily by the Rossi X-ray Timing Explorer (RXTE) during most of its 8-month outburst in 2003. We present a detailed spectral analysis and a supporting timing analysis of all of these data,…

We describe observations of the 2003 outburst of the hard-spectrum X-ray transient 4U 1901+03 with the Rossi X-ray Timing Explorer. The outburst was first detected in 2003 February by the All-Sky Monitor, and reached a peak 2.5-25 keV flux…

Astrophysics · Physics 2009-11-11 Duncan K. Galloway , Zhongxiang Wang , Edward H. Morgan

We present the results of our spectral and timing analysis of the emission from the transient X-ray pulsar XTE J1946+274 based on the simultaneous NuSTAR and Swift/XRT observations in the broad energy range 0.3-79 keV carried out in June…

High Energy Astrophysical Phenomena · Physics 2021-10-12 A. S. Gorban , S. V. Molkov , S. S. Tsygankov , A. A. Lutovinov

XTE J1810-197 is the first transient Anomalous X-ray Pulsar ever discovered. Its highly variable X-ray flux allowed us to study the timing and spectral emission properties of a magnetar candidate over a flux range of about two orders of…

High Energy Astrophysical Phenomena · Physics 2009-11-13 F. Bernardini , G. L. Israel , S. Dall'Osso , L. Stella , N. Rea , S. Zane , R. Turolla , R. Perna , M. Falanga , S. Campana , D. Götz , S. Mereghetti , A. Tiengo

Using X-ray data from the Rossi X-Ray Timing Explorer (RXTE), we carried out pulse timing analysis of the transient X-ray pulsar SAX J2103.5+4545. An outburst was detected by All Sky Monitor (ASM) October 25 1999 and reached a peak X-ray…

Astrophysics · Physics 2009-10-31 A. Baykal , M. Stark , J. Swank

The Be/X-ray binary pulsar RX J0440.9+4431 underwent a giant outburst in late 2022 and lasted three months. The Insight-HXMT has observed this source at several instances of the entire outburst in 2022-2023. We used these bright outburst…

High Energy Astrophysical Phenomena · Physics 2025-09-17 Prahlad R. Epili , Wei Wang

We analyze the observations of the X-ray pulsar KS 1947+300 performed by the INTEGRAL and RXTE observatories over a wide (3-100 keV) X-ray energy range. The shape of the pulse profile was found to depend on the luminosity of the source.…

Astrophysics · Physics 2009-11-10 S. S. Tsygankov , A. A. Lutovinov

We present here the preliminary results of the study of the fluorescent iron line emission from X-ray pulsars with Be companions. We propose to use properties of this emission to investigate the spatial distribution and physical conditions…

High Energy Astrophysical Phenomena · Physics 2010-02-10 S. Tsygankov , A. Lutovinov

In 1993-1994 a series of observations of the X-ray pulsar GX 301-2 by HEXE onboard Mir-Kvant was made. A period of pulsations was measured (it varied between 675 and 678 s) and pulse profiles in different energy bands were produced. The…

We analyze the observations of the transient X-ray pulsar 4U 0115+63 with the RXTE and INTEGRAL observatories in a wide X-ray (3-100 keV) energy band during its intense outbursts in 1999 and 2004. The energy of the fundamental harmonic of…

Astrophysics · Physics 2009-06-23 S. S. Tsygankov , A. A. Lutovinov , E. M. Churazov , R. A. Sunyaev

The long-term observations of the Galactic Centre as well as the Galactic anti-Centre regions in hard X-rays (10-300 keV) were made in experiments on board Prognoz-9 satellite and "Mir" orbital station (GRIF experiment). Some transient…

Astrophysics · Physics 2007-05-23 M. I. Kudryavtsev , S. I. Svertilov , V. V. Bogomolov

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

We probe the properties of the transient X-ray pulsar MAXI J1409$-$619 through \textit{RXTE} and \textit{Swift} follow up observations of the outburst in 2010. We are able to phase connect the pulse arrival times for the 25 days episode…

High Energy Astrophysical Phenomena · Physics 2020-06-17 Ç. K. Dönmez , M. M. Serim , S. Ç. İnam , Ş. Şahiner , D. Çerri-Serim , A. Baykal

We present two observational campaigns performed with the RXTE satellite on the black hole transient H 1743-322. The source was observed in outburst on two separate occasions between October-November 2008 and May-July 2009. We have carried…

High Energy Astrophysical Phenomena · Physics 2015-05-19 S. Motta , T. Muñoz-Darias , T. Belloni

In this Letter we present results from INTEGRAL and RXTE observations of the spectral and timing behavior of the High Mass X-ray Binary A 0535+26 during its August/September 2005 normal (type I) outburst with an average flux…

We report timing and spectral properties of the transient Be X-ray pulsar EXO 053109--6609.2 studied using observations made with the ASCA and BeppoSAX observatories. Though there must have been at least one spin-down episode of the pulsar…

Astrophysics · Physics 2009-11-10 B. Paul , S. N. A. Jaaffery , S. Naik , P. C. Agrawal

(Abridged) We present a multi-epoch spectral study of the Transient Anomalous X-ray Pulsar XTE J1810-197 obtained with the XMM X-ray telescope. Four observations taken over the course of a year reveal strong spectral evolution as the source…

Astrophysics · Physics 2009-11-13 E. V. Gotthelf , J. P. Halpern

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…

High Energy Astrophysical Phenomena · Physics 2022-03-30 P. Reig , R. C. Ma , L. Tao , S. Zhang , S. N. Zhang , V. Doroshenko

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…

High Energy Astrophysical Phenomena · Physics 2018-07-25 Shivangi Gupta , Sachindra Naik , Gaurava K. Jaisawal , Prahlad R. Epili

The decline of the high mass X-ray transient V0332+53 during the Dec. 2004 to Feb. 2005 outburst is analysed from the data recorded by INTEGRAL. The flux is shown to decrease exponentially until 2005 Feb. 10, with a decay time scale of \~30…