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相关论文: The INTEGRAL source IGR J16328-4726: a High Mass X…

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We report the association of the INTEGRAL source IGR J18027-2016 with the BeppoSAX source SAX J1802.7-2017. IGR J18027-2016 is seen to be a weak, persistent source by the IBIS/ISGRI instrument on board INTEGRAL with an average source count…

Of the 21 new sources that INTEGRAL discovered up to Feb. 1, 2004, five were detected with the BeppoSAX Wide Field Cameras at earlier times. IGR J16320-4751 appears to be a persistently active X-ray source which hints at a supergiant…

天体物理学 · 物理学 2007-05-23 Jean in 't Zand , John Heise , Pietro Ubertini , Angela Bazzano , Craig Markwardt

The hard X-ray source IGRJ11215-5952, discovered with INTEGRAL during a brief outburst in 2005, has been proposed as a new member of the class of Supergiant Fast X-ray Transients. Analysing archival INTEGRAL observations of the source…

天体物理学 · 物理学 2008-11-26 Lara Sidoli , Ada Paizis , Sandro Mereghetti

We report the results of a high-energy multi-instrumental campaign with INTEGRAL, RXTE, and Swift of the recently discovered INTEGRAL source IGR J19294+1816. The Swift/XRT data allow us to refine the position of the source to RA= 19h 29m…

高能天体物理现象 · 物理学 2015-05-14 J. Rodriguez , J. A. Tomsick , A. Bodaghee , J. -A. Zurita Heras , S. Chaty , A. Paizis , S. Corbel

SAX J1818.6-1703 is a flaring transient X-ray source serendipitously discovered by BeppoSAX in 1998 during an observation of the Galactic centre. The source was identified as a High-Mass X-ray Binary with an OB SuperGiant companion.…

天体物理学 · 物理学 2009-11-13 J. A. Zurita Heras , S. Chaty

Context: The transient hard X-ray source IGR J11321-5311 was discovered by INTEGRAL on June 2005, during observations of the Crux spiral arm. To date, this is the only detection of the source to be reported by any X/gamma-ray mission. Aims:…

天体物理学 · 物理学 2009-11-13 V. Sguera , A. Bazzano , A. J. Bird , A. B. Hill , A. J. Dean , L. Bassani , A. Malizia , P. Ubertini

We present the transient nature of INTEGRAL source IGR J17285-2922, identified from a single period of activity during an IBIS/ISGRI Galactic Centre Deep Exposure in September 2003. The source has a maximum detection significance of 14…

We present an INTEGRAL data analysis of the X-ray transient \object{SAX J2103.5+4545} during two outbursts detected in December 2002. The INTEGRAL coordinates and error circle agree with the position of the recently proposed optical…

天体物理学 · 物理学 2009-11-10 P. Blay , P. Reig , S. Martinez Nunez , A. Camero , P. Connell , V. Reglero

The hard X-ray source IGRJ11215-5952 has been discovered with INTEGRAL during a short outburst in 2005 and proposed as a new member of the class of supergiant fast X-ray transients. We analysed INTEGRAL public observations of the source…

天体物理学 · 物理学 2009-11-11 L. Sidoli , A. Paizis , S. Mereghetti

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 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

The X-ray source SAXJ1712.6-3739 is a very weak Low Mass X-ray Binary discovered in 1999 with BeppoSAX and located in the Galactic Center. This region has been deeply investigated by the INTEGRAL satellite with an unprecedented exposure…

天体物理学 · 物理学 2009-11-13 Mariateresa Fiocchi , Angela Bazzano , Pietro Ubertini , Giovanni De Cesare

We have characterized the typical temporal behaviour of the bright X-ray flares detected from the three Supergiant Fast X-ray Transients showing the most extreme transient behaviour (XTEJ1739-302, IGRJ17544-2619, SAXJ1818.6-1703). We focus…

高能天体物理现象 · 物理学 2016-02-03 L. Sidoli , A. Paizis , K. Postnov

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

We report new X-ray results from the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL), Swift, Chandra, and XMM-Newton observations of the hitherto poorly studied unidentified X-ray transient IGR J17419-2802. We studied in detail…

高能天体物理现象 · 物理学 2024-09-10 V. Sguera , L. Sidoli

The discovery of the X-ray source IGR J17252-3616 by INTEGRAL was reported on 9 February 2004. Regular monitoring by INTEGRAL shows that IGR J17252-3616 is a persistent hard X-ray source with an average count rate of 0.96 counts/s (~6.4…

We report on a broad-band X-ray study (0.5-60 keV) of the poorly known candidate Supergiant Fast X-ray Transient (SFXT) IGR J18462-0223, and on optical and near-infrared (NIR) followup observations of field objects. The out-of-outburst…

高能天体物理现象 · 物理学 2015-06-15 V. Sguera , S. P. Drave , L. Sidoli , N. Masetti , R. Landi , A. J. Bird , A. Bazzano

INTEGRAL regularly scans the Galactic plane to search for new objects and in particular for absorbed sources with the bulk of their emission above 10-20 keV. The first new INTEGRAL source was discovered on 2003 January 29, 0.5 degree from…

We report on the results of INTEGRAL observations of the neutron star low mass X-ray binary SAX J1810.8-2609 during its latest active phase in August 2007. The current outburst is the first one since 1998 and the derived luminosity is…

The supergiant fast X-ray transient IGR J08408-4503 was discovered by INTEGRAL on May 15, 2006, during a bright flare. The source shows sporadic recurrent short bright flares, reaching a peak luminosity of 10^36 erg s^-1 within less than…

天体物理学 · 物理学 2011-02-11 D. Gotz , M. Falanga , F. Senziani , A. De Luca , S. Schanne , A. von Kienlin
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