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相关论文: INTEGRAL observations of recurrent fast X-ray tran…

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Context: AXJ1845.0-0433 was discovered by ASCA in 1993 during fast outburst activity characterized by several flares on short timescales. Up to now, the source was not detected again by any X-ray mission. Its optical counterpart is…

SFXTs are a new class of HMXB unveiled by INTEGRAL. They are extreme systems characterised by very short outbursts (a few hours) and extreme X-ray luminosity dynamic ranges (~10^{4}). Ten confirmed systems are currently known and have shown…

高能天体物理现象 · 物理学 2011-05-04 S. P. Drave , A. J. Bird , D. J. Clark , V. A. McBride , A. B. Hill , V. Sguera , S. Scaringi , A. Bazzano , L. J. Townsend

We studied the soft-X-ray emission of five hard-X sources: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703 and IGR J17348-2045. These sources are: a confirmed supergiant high mass X-ray binary (IGR J08262-3736);…

高能天体物理现象 · 物理学 2013-03-20 L. Pavan , E. Bozzo , C. Ferrigno , M. Falanga , S. Campana , S. Paltani , L. Stella , R. Walter

The unidentified source IGR J16328-4726 was covered with INTEGRAL observations for a long period (~9.8Ms) and was undetectable for most of the time while showing a very recurrent micro-activity with a duration from tens minutes to several…

高能天体物理现象 · 物理学 2015-05-20 M. Fiocchi , V. Sguera , A. Bazzano , L. Bassani , A. J. Bird , L. Natalucci , P. Ubertini

IGR J16479-4514 is a Supergiant Fast X-ray Transient (SFXT), a new class of High Mass X-ray Binaries, whose number is rapidly growing thanks to the observations of the Galactic plane performed with the INTEGRAL satellite. IGR J16479-4514…

天体物理学 · 物理学 2009-11-13 P. Romano , L. Sidoli , V. Mangano , S. Vercellone , J. A. Kennea , G. Cusumano , H. A. Krimm , D. N. Burrows , N. Gehrels

After the first nine years of INTEGRAL operational life, the discovery of new sources and source types, a large fraction of which are highly transient or highly absorbed, is certainly one of the most compelling results and legacies of…

高能天体物理现象 · 物理学 2019-08-14 Mariateresa Fiocchi , Lorenzo Natalucci

Supergiant Fast X-ray Transients (SFXTs) are a sub-class of High Mass X-ray Binaries (HMXBs) associated with OB supergiant companions and displaying transient X-ray activity. This behaviour is quite surprising since HMXBs hosting…

Context. On April 14, 2009, the AGILE satellite detected a {\gamma}-ray flare from an unknown transient source. Subsequent X-ray follow-up observations with Swift and INTEGRAL identified the supergiant fast X-ray transient (SFXT) IGR…

Fast X-ray transients (FXTs) are flashes of X-rays that last for a few hundreds of seconds to a few hours. An enigmatic population of these transients that did not have a clear origin has been known for several decades, mostly found…

高能天体物理现象 · 物理学 2026-01-22 Murray Brightman , Joahan Castañeda Jaimes , Daniel Stern , Brian Grefenstette

Very Faint X-ray Transients (VFXTs) are a class of X-ray binary systems that exhibit occasional outbursts with peak X-ray luminosities (L_X< 1e36 erg s^-1) much lower than typical X-ray transients. On 22nd February 2024, during its daily…

In this paper, we report on the available X-ray data collected by INTEGRAL, Swift, and XMM-Newton during the first outburst of the INTEGRAL transient IGR J17451-3022, discovered in 2014 August. The monitoring observations provided by the…

高能天体物理现象 · 物理学 2016-04-13 E. Bozzo , P. Pjanka , P. Romano , A. Papitto , C. Ferrigno , S. Motta , A. A. Zdziarski , F. Pintore , T. Di Salvo , L. Burderi , D. Lazzati , G. Ponti , L. Pavan

IGR J19140+098 was discovered during the early INTEGRAL observations of GRS1915+105 in March 2003. The following observations by INTEGRAL and RXTE show significant variability on various time scales from 100s to 1ks, but no pulsations. The…

天体物理学 · 物理学 2007-05-23 C. Cabanac , J. Rodriguez , P. O Petrucci , G. Henri , D. Hannikainen , P. Durouchoux

We present results of spectral and timing analysis of the fast X-ray transient XTE J1901+014 based on data of the RXTE and INTEGRAL observatories. With the INTEGRAL/ISGRI the source was detected at a significance level of 20$\sigma$ with…

天体物理学 · 物理学 2007-05-23 D. I. Karasev , A. A. Lutovinov , S. A. Grebenev

IGRJ19294+1816 was discovered by INTEGRAL in 2009 during a bright X-ray outburst and was classified as a possible Be X-ray binary or supergiant fast X-ray transient. On 2010 October 28, the source displayed a second X-ray outburst and a 2…

高能天体物理现象 · 物理学 2015-05-28 E. Bozzo , C. Ferrigno , M. Falanga , R. Walter

In the past few years, a new class of High Mass X-Ray Binaries (HMXRB) has been claimed to exist, the Supergiant Fast X-ray Transients (SFXT). These are X-ray binary systems with a compact companion orbiting a supergiant star which show…

Supergiant Fast X-ray Transients are a class of Galactic High Mass X-ray Binaries with supergiant companions. Their extreme transient X-ray flaring activity was unveiled thanks to INTEGRAL/IBIS observations. The SFXTs dynamic range, with…

高能天体物理现象 · 物理学 2013-02-01 Lara Sidoli

IGR J18483-0311 is a poorly known transient hard X-ray source discovered by INTEGRAL during observations of the Galactic Center region performed between 23--28 April 2003. Aims: To detect new outbursts from IGR J18483-0311 using INTEGRAL…

天体物理学 · 物理学 2009-11-13 V. Sguera , A. B. Hill , A. J. Bird , A. J. Dean , A. Bazzano , P. Ubertini , N. Masetti , R. Landi , A. Malizia , D. J. Clark , M. Molina

XTE J1739-302 is a transient X-ray source with unusually short outbursts, lasting on the order of hours. Here we give a summary of X-ray observations we have made of this object in outburst with the Rossi X-ray Timing Explorer (RXTE) and at…

天体物理学 · 物理学 2009-11-13 D. M. Smith , W. A. Heindl , C. B. Markwardt , J. H. Swank , I. Negueruela , T. E. Harrison , L. Huss

We report the discovery of a high-energy transient with the IBIS/ISGRI detector on board the INTEGRAL observatory. The source, namely IGR J00291+5934, was first detected on 2nd December 2004 in the routine monitoring of the IBIS/ISGRI…

We report results from an investigation at hard X-rays (above 18 keV) and soft X-rays (below 10 keV) of a sample of X-ray transients located on the Galactic plane and detected with the bursticity method, as reported in the latest 1,000…

高能天体物理现象 · 物理学 2020-01-22 V. Sguera , L. Sidoli , A. J. Bird , A. Paizis , A. Bazzano