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The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) is discovering a large number of new hard X-ray sources, many of them being HMXBs. The identification and spectral characterization of their optical/infrared counterparts is a…

高能天体物理现象 · 物理学 2015-05-18 E. Nespoli , J. Fabregat , R. E. Mennickent

Supergiant high mass X-ray binaries (SGXBs) are believed to be rare objects, as stars in the supergiant phase have a very short lifetime and to date only about a dozen of them have been discovered. They are known to be persistent and bright…

Since it started observing the sky, the INTEGRAL satellite has discovered new categories of high mass X-ray binaries (HMXB) in our Galaxy. These observations raise important questions on the formation and evolution of these rare and…

高能天体物理现象 · 物理学 2015-06-17 Alexis Coleiro , Sylvain Chaty , Juan A. Zurita Heras , Farid Rahoui , John A. Tomsick

We analyzed in a systematic way the public INTEGRAL observations spanning from December 2002 to September 2016, to investigate the hard X-ray properties of about 60 High Mass X-ray Binaries (HMXBs). We considered both persistent and…

高能天体物理现象 · 物理学 2018-09-12 Lara Sidoli , Adamantia Paizis

The INTEGRAL archive developed at INAF-IASF Milano with the available public observations from late 2002 to 2016 is investigated to extract the X-ray properties of 58 High Mass X-ray Binaries (HMXBs). This sample consists of sources hosting…

高能天体物理现象 · 物理学 2020-02-19 Lara Sidoli , Adamantia Paizis

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

We summarize the results of our long-running campaign to help understand the nature of high-mass X-ray binaries (HMXBs), emphasizing recent Suzaku observations of IGR J16207-5129 and IGR J17391-3021. Thanks to the expanding ranks of HMXBs…

高能天体物理现象 · 物理学 2011-02-18 Arash Bodaghee , John A. Tomsick , Jerome Rodriguez

Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in the course of being unveiled by means of…

天体物理学 · 物理学 2009-11-13 Farid Rahoui , Sylvain Chaty , Pierre-Olivier Lagage , Eric Pantin

Supergiant Fast X-ray Transients (SFXTs) are one of the most intriguing (and unexpected) results of the INTEGRAL mission. They are a new class of High Mass X-ray Binaries involving about 20 sources to date, with 8 firmly identified SFXTs…

天体物理仪器与方法 · 物理学 2010-01-20 L. Sidoli , V. Sguera , A. Bazzano , P. Ubertini

We report on Suzaku observations of four unidentified sources from the INTEGRAL and Swift BAT Galactic plane surveys. All the sources have a large neutral hydrogen column density and are likely members of an emerging class of heavily…

天体物理学 · 物理学 2011-02-11 D. C. Morris , R. K. Smith , C. B. Markwardt , R. F. Mushotzky , J. Tueller , T. R. Kallman , K. S. Dhuga

We have analyzed in a systematic way about nine years of INTEGRAL data (17-100 keV) focusing on Supergiant Fast X-ray Transients (SFXTs) and three classical High Mass X-ray Binaries (HMXBs). Our approach has been twofold: image based…

高能天体物理现象 · 物理学 2014-03-05 A. Paizis , L. Sidoli

Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources:…

高能天体物理现象 · 物理学 2016-10-05 P. Romano , E. Bozzo , P. Esposito , B. Sbarufatti , F. Haberl , G. Ponti , P. D'Avanzo , L. Ducci , A. Segreto , C. Jin , N. Masetti , M. Del Santo , S. Campana , V. Mangano

Supergiant Fast X-ray Transients (SFXTs) are a new class of HMXBs discovered thanks to the monitoring of the Galactic plane performed with the INTEGRAL satellite in the last 5 years. These sources display short outbursts (significantly…

We combine infrared spectra in the I, J, H and K bands together with JHK photometry to characterize the spectral type, luminosity class and distance to the infrared counterparts to five INTEGRAL sources. For SAX J18186-1703 and IGR…

太阳与恒星天体物理 · 物理学 2015-05-14 J. M. Torrejón , I. Negueruela , D. M. Smith , T. E. Harrison

Since its launch, the X-ray and gamma-ray observatory INTEGRAL satellite has revealed a new class of high-mass X-ray binaries (HMXB) displaying fast flares and hosting supergiant companion stars. Optical and infrared (OIR) observations in a…

INTEGRAL monitoring of the Galactic Plane is revealing a growing number of recurrent X-ray transients, characterised by short outbursts with very fast rise times (~ tens of minutes) and typical durations of a few hours. Here we show that…

天体物理学 · 物理学 2007-05-23 Ignacio Negueruela , David M. Smith , Pablo Reig , Sylvain Chaty , Jose Miguel Torrejon

Since its launch, the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) satellite has discovered hundreds of X-ray sources, many of which lack proper classification. This mission also led to the discovery of new categories of high…

高能天体物理现象 · 物理学 2022-10-24 Tristan Bouchet , Sylvain Chaty , Francis Fortin , John A. Tomsick

INTEGRAL monitoring of the Galactic Plane in the last 5 years revealed a new subclass of High Mass X-ray Binaries (HMXBs), the Supergiant Fast X-ray Transients (SFXTs). They display flares lasting from minutes to hours, with peak luminosity…

天体物理学 · 物理学 2010-04-30 L. Ducci , L. Sidoli , A. Paizis , S. Mereghetti

The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in X-rays below 2 keV. On 2003, February, 23--25…

天体物理学 · 物理学 2007-05-23 Sylvain Chaty , Philippe Filliatre

A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among these sources, two…

天体物理学 · 物理学 2007-10-02 Sylvain Chaty
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