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The black-hole X-ray binary transient GRO J1655-40 underwent an outburst beginning in early 2005. We present the results of our multi-wavelength observational campaign to study the early outburst spectral and temporal evolution, which…

天体物理学 · 物理学 2008-11-26 N. Shaposhnikov , J. Swank , C. R. Shrader , M. Rupen , V. Beckmann , C. B. Markwardt , D. A. Smith

On March 2003, IBIS, the gamma-ray imager on board the INTEGRAL satellite, detected an outburst from a new source, IGR J17464-3213, that turned out to be a HEAO-1 transient, H1743-322. In this paper we report on the high energy behaviour of…

Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the onset of its X-ray outburst in January,…

天体物理学 · 物理学 2009-11-11 Sylvain Chaty , Nicolas Bessolaz

We evaluate 0.03-20 Hz power spectra of the bright black hole binary Cyg X-1 obtained from non-deconvolved INTEGRAL-ISGRI event data. The ISGRI power spectra are compared to contemporary RXTE-PCA ones in the same hard X-ray energy band of…

天体物理学 · 物理学 2009-11-11 K. Pottschmidt , J. Wilms , M. A. Nowak , S. Larsson , A. A. Zdziarski , G. G. Pooley

One of the most straightforward ways to explain the hard X-ray spectra observed in X-ray binaries is to assume that comptonization of soft photons from the accretion disk is occurring. The region where this process takes place, called the…

高能天体物理现象 · 物理学 2021-03-31 Paulo Eduardo Stecchini , Jurandi Leão , Manuel Castro , Flavio D'Amico

We present a detailed spectral analysis of the Black Hole Binary XTE J1752-223 in the hard state of its 2009 outburst. Regular monitoring of this source by RXTE provided high signal-to-noise spectra along the outburst rise and decay. During…

Galactic black hole transients show many interesting phenomena during outburst decays. We present simultaneous X-ray (RXTE, Swift, and INTEGRAL), and optical/near-infrared (O/NIR) observations (SMARTS) of the X-ray transient XTE J1752-223…

高能天体物理现象 · 物理学 2015-06-15 Y. Y. Chun , T. Dinçer , E. Kalemci , T. Güver , J. A. Tomsick , M. M. Buxton , C. Brocksopp , S. Corbel , A. Cabrera-Lavers

We present the analysis of an extended \textit{INTEGRAL} dataset of the high-mass microquasar Cygnus X-1. We first classify, in a model-independent way, all the \textit{INTEGRAL} individual pointings taken between 2003 and 2016 in three…

高能天体物理现象 · 物理学 2018-11-12 Floriane Cangemi , Jérôme Rodriguez , Victoria Grinberg , Philippe Laurent , Joern Wilms

We studied spectra for 34 accretion-powered X-ray and one millisecond pulsars that were within the field of view of the INTEGRAL observatory over two years (December 2002 - January 2005) of its in-orbit operation and that were detected by…

天体物理学 · 物理学 2007-05-23 E. V. Filippova , S. S. Tsygankov , A. A. Lutovinov , R. A. Sunyaev

We report results from joint NuSTAR, Swift and XMM-Newton observations of the newly discovered black hole X-ray binary candidate Swift J1658.2-4242 in the intermediate state. We observe a peculiar event in this source, with its X-ray flux…

Studies of the long-term spectral variations have been used to constrain the emission processes of black hole candidates. However, a common scenario which is able to explain the emission from soft to hard X-rays has been proposed only…

高能天体物理现象 · 物理学 2013-02-26 Manuel Castro , Taís Maiolino , Flavio D'Amico , Jörn Wilms , Katja Pottschmidt , João Braga

LS 5039/RX J1826.2-1450 is one of the few High Mass X-ray binary systems from which radio and high energy TeV emission has been observed. Moreover, variability of the TeV emission with orbital period was detected. We investigate the hard…

天体物理学 · 物理学 2009-11-13 A. D. Hoffmann , D. Klochkov , A. Santangelo , D. Horns , A. Segreto , R. Staubert , G. Puehlhofer

We report results of a one-year monitoring of the low mass X-ray binary (LMXB) source (atoll type) 4U 1728-34 with INTEGRAL and RXTE. Three time intervals were covered by INTEGRAL, during which the source showed strong spectral evolution.…

高能天体物理现象 · 物理学 2015-05-27 A. Tarana , T. Belloni , A. Bazzano , M. Méndez , P. Ubertini

We present first results from contemporaneous observations of Cygnus X-1 with INTEGRAL and RXTE, made during INTEGRAL's performance verification phase in 2002 November and December. Consistent with earlier results, the 3-250 keV data are…

During the June 2015 outburst of the black hole binary V404 Cyg, rapid changes in the X-ray brightness and spectra were common. The INTEGRAL monitoring campaign detected spectacular Eddington-limited X-ray flares, but also rapid variations…

高能天体物理现象 · 物理学 2020-02-19 J. J. E. Kajava , C. Sánchez-Fernández , J. Alfonso-Garzón , S. E. Motta , A. Veledina

We report on high energy observations of IGR J19140+0951 performed with RXTE on three occasions in 2002, 2003 and 2004, and INTEGRAL during a very well sampled and unprecedented high energy coverage of this source from early-March to…

天体物理学 · 物理学 2009-11-10 J. Rodriguez , C. Cabanac , D. C. Hannikainen , V. Beckmann , S. E. Shaw , J. Schultz

We report on a recent bright outburst from the new X-ray binary transient MAXI J1631-479, observed in January 2019. In particular, we present the 30-200 keV analysis of spectral transitions observed with INTEGRAL/IBIS during its Galactic…

高能天体物理现象 · 物理学 2020-01-22 M. Fiocchi , F. Onori , A. Bazzano , A. J. Bird , A. Bodaghee , P. A. Charles , V. A. Lepingwell , A. Malizia , N. Masetti , L. Natalucci , P. Ubertini

We report MAXI and Swift observations of short-term spectral softenings of the galactic black-hole X-ray binary Swift J1753.5-0127 in the low/hard state. These softening events are characterized by a simultaneous increase of soft X-rays…

We present preliminary results of observations of X-ray pulsar SAX J2103.5+4545 with INTEGRAL observatory in Dec 2002. Maps of this sky region in energy bands 3-10, 15-40, 40-100 and 100-200 keV are presented. The source is significantly…

天体物理学 · 物理学 2009-11-07 A. Lutovinov , S. Molkov , M. Revnivtsev

We present the results of Rossi X-ray Timing Explorer observations of GS 1354-644 during a modest outburst in 1997-1998. The source is one of a handful of black hole X-ray transients that are confirmed to be recurrent in X-rays. A 1987…