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相关论文: The 2013 outburst of a transient very faint X-ray …

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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…

Recent X-ray and radio observations have identified a transient low-mass X-ray binary (LMXB) located only 0.1 pc in projection from the Galactic center, CXOGC J174540.0-290031. In this paper, we report the detailed analysis of X-ray and…

天体物理学 · 物理学 2009-02-18 M. P. Muno , J. R. Lu , F. K. Baganoff , W. N. Brandt , G. P. Garmire , A. M. Ghez , S. D. Hornstein , M. R. Morris

During the observation of the Galactic-center field by the INTEGRAL observatory on September 9, 2003, the IBIS/ISGRI gamma-ray telescope detected a short (several-hours-long) intense (~380 mCrab at the peak) outburst of hard radiation from…

天体物理学 · 物理学 2009-11-13 S. A. Grebenev , R. A. Sunyaev

We report on multi-band observations of the transient source Swift J0840.7-3516, which was detected in outburst in 2020 February by the Neil Gehrels Swift Observatory. The outburst episode lasted just ~5 days, during which the X-ray…

高能天体物理现象 · 物理学 2021-06-09 F. Coti Zelati , A. de Ugarte Postigo , T. D. Russell , A. Borghese , N. Rea , P. Esposito , G. L. Israel , S. Campana

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

CONTEXT - Transient low-mass X-ray binaries (LMXBs) often show outbursts lasting typically a few-weeks and characterized by a high X-ray luminosity ($L_{x} \approx 10^{36}-10^{38}$ erg/sec), while for most of the time they are found in…

Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries associated with OB supergiant companions and characterised by an X-ray flaring behaviour whose dynamical range reaches 5 orders of magnitude on timescales of a few…

高能天体物理现象 · 物理学 2015-03-25 P. Romano , E. Bozzo , V. Mangano , P. Esposito , G. Israel , A. Tiengo , S. Campana , L. Ducci , C. Ferrigno , J. A. Kennea

We report on continued monitoring observations of the Galactic center carried out by the X-ray telescope aboard the Swift satellite in 2008 and 2009. This campaign revealed activity of the five known X-ray transients AX J1745.6-2901, CXOGC…

高能天体物理现象 · 物理学 2015-05-19 N. Degenaar , R. Wijnands

We present Chandra/ACIS observations of the bursting X-ray transient SAX J1747.0-2853 performed on 18 July 2001. We detected a bright source at the position of R.A = 17^h 47^m 02.60^s and Dec. = -28 52' 58.9'' (J2000.0; with a 1 sigma error…

天体物理学 · 物理学 2009-11-07 Rudy Wijnands , J. M. Miller , Q. Daniel Wang

XMMSL1 J171900.4-353217 is a very-faint X-ray transient that was discovered in 2010 March when it exhibited an outburst. We report on 7 observations, obtained with the X-Ray Telescope (XRT) aboard the Neil Gehrels {\it{Swift}} Observatory…

高能天体物理现象 · 物理学 2024-10-01 O. Ahmed , N. Degenaar , R. Wijnands , M. Armas Padilla

We present two years of intense Swift monitoring of three SFXTs, IGR J16479-4514, XTE J1739-302, and IGR J17544-2619 (since October 2007). Out-of-outburst intensity-based X-ray (0.3-10keV) spectroscopy yields absorbed power laws with by…

Swift observed an outburst from the supergiant fast X-ray transients (SFXT) AX J1841.0-0536 on 2010 June 5, and followed it with XRT for 11 days. The X-ray light curve shows an initial flare followed by a decay and subsequent increase, as…

Details of the discovery of a new X-ray source, IGR J18462-0223, on October 12, 2007, during a short (several hours), intense (~ 35 mCrab at the peak) outburst of hard radiation by the IBIS/ISGRI gamma-ray telescope onboard the INTEGRAL…

高能天体物理现象 · 物理学 2015-05-20 S. A. Grebenev , R. A. Sunyaev

IGR J17544-2619 and XTE J1739-302 are considered the prototypical sources of the new class of High Mass X-ray Binaries, the Supergiant Fast X-ray Transients (SFXTs).These sources were observed during bright outbursts on 2008 March 31 and…

We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004 of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at only 2.9" from SgrA*. We report the discovery of sharp and…

天体物理学 · 物理学 2009-11-11 D. Porquet , N. Grosso , G. Belanger , A. Goldwurm , F. Yusef-Zadeh , R. S. Warwick , P. Predehl

On 28 February 2007 a new outburst of the previously known transient source XTE J1856+053 was detected with RXTE/ASM. We present here the results of an XMM-Newton (0.5-10.0 keV) Target of Opportunity observation performed on 14 March 2007,…

天体物理学 · 物理学 2011-08-31 G. Sala , J. Greiner , M. Ajello , N. Primak

We have analysed in detail the discovery measurements of the X-ray burster SAX J1750.8-2900 by the Wide Field Cameras on board BeppoSAX in spring 1997, at a position ~1.2 degrees off the Galactic Centre. The source was in outburst on March…

天体物理学 · 物理学 2009-10-31 L. Natalucci , R. Cornelisse , A. Bazzano , M. Cocchi , P. Ubertini , J. Heise , J. J. M. in 't Zand , E. Kuulkers

We report on a thermonuclear (type-I) X-ray burst that was detected from the neutron star low-mass X-ray binary SAX J1810.8-2609 in 2007 with Swift. This event was longer (~20 min) and more energetic (a radiated energy of Eb~6.5E39 erg)…

高能天体物理现象 · 物理学 2015-06-11 N. Degenaar , R. Wijnands

We report the first broad-band (0.5-150 keV) simultaneous X-ray observations of the very faint X-ray transient IGRJ17285-2922/XTEJ1728-295 performed with XMM-Newton and INTEGRAL satellites during its last outburst, started on 2010, August…

高能天体物理现象 · 物理学 2015-05-27 L. Sidoli , A. Paizis , S. Mereghetti , D. Gotz , M. Del Santo

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
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