English
Related papers

Related papers: IGRJ16479-4514: the first eclipsing supergiant fas…

200 papers

IGR J01583+6713 is a new transient source discovered by the INTEGRAL/IBIS hard X-ray surveys. Optical observations suggested that it should be a high mass X-ray binary, but its nature is still unclear. We used the INTEGRAL/IBIS data to…

High Energy Astrophysical Phenomena · Physics 2015-05-14 W. Wang

Context : A 1000-s flare from a new hard X-ray transient, IGR J08408-4503, was observed by INTEGRAL on May 15, 2006 during the real-time routine monitoring of IBIS/ISGRI images performed at the INTEGRAL Science Data Centre. The flare,…

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…

High Energy Astrophysical Phenomena · Physics 2017-07-19 M. Matranga , A. Papitto , T. Di Salvo , E. Bozzo , D. F. Torres , R. Iaria , L. Burderi , N. Rea , D. de Martino , C. Sanchez-Fernandez , A. F. Gambino , C. Ferrigno , L. Stella

IGR J18214-1318, a Galactic source discovered by the International Gamma-Ray Astrophysics Laboratory, is a high-mass X-ray binary (HMXB) with a supergiant O-type stellar donor. We report on the XMM-Newton and NuSTAR observations that were…

The Galactic center region was observed with the XRISM X-ray observatory during the performance verification phase in 2024 and a point-like X-ray source was detected with the X-ray imager Xtend at a position of (RA, Dec)=(17h46m10.8s,…

IGR J18179-1621 is an obscured accreting X-ray pulsar discovered by INTEGRAL on 2012 February 29. We report on our 20 ksec Chandra-High Energy Transmission Gratings Spectrometer observation of the source performed on 2012 March 17, on two…

High Energy Astrophysical Phenomena · Physics 2015-06-05 M. A. Nowak , A. Paizis , J. Rodriguez , S. Chaty , M. Del Santo , V. Grinberg , J. Wilms , P. Ubertini , R. Chini

We report on a quasi-periodic variation at $\sim1$ Hz during a fast X-ray outburst of a high-mass X-ray binary MAXI J0709$-$159 / LY CMa observed by the Neutron-star interior composition explorer (NICER). The new X-ray transient MAXI…

AX J1949.8+2534 is a candidate supergiant fast X-ray transient (SFXT) observed in outburst by INTEGRAL (IGR J19498+2534). We report on the results of six Neil Gehrels Swift-XRT, one Chandra, and one NuSTAR observation of the source. We find…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Jeremy Hare , Jules P. Halpern , Maica Clavel , Jonathan E. Grindlay , Farid Rahoui , John A. Tomsick

On 2008 May 14, the Burst Alert Telescope aboard the Swift mission triggered on a type-I X-ray burst from the previously unclassified ROSAT object 1RXH J173523.7-354013, establishing the source as a neutron star X-ray binary. We report on…

In this paper we report on the spectral analysis of seven X-ray transients, which were found to be active during a monitoring campaign of the Galactic center carried out in 2006 and 2007 using the X-ray telescope aboard the Swift satellite.…

Astrophysics · Physics 2009-11-13 N. Degenaar , R. Wijnands

We report on a Chandra grating observation of the recently discovered hard X-ray transient IGR J17497-2821. The observation took place about two weeks after the source discovery at a flux level of about 20 mCrab in the 0.8-8 keV range. We…

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…

Astrophysics · Physics 2007-05-23 Jean in 't Zand , John Heise , Pietro Ubertini , Angela Bazzano , Craig Markwardt

We report on the identification of the new Galactic Center (GC) transient Swift J174540.7-290015 as a likely low mass X-ray binary (LMXB) located at only 16 arcsec from Sgr A*. This transient was detected on 2016 February 6th during the…

High Energy Astrophysical Phenomena · Physics 2016-06-15 G. Ponti , C. Jin , B. De Marco , N. Rea , A. Rau , F. Haberl , F. Coti Zelati , E. Bozzo , C. Ferrigno , G. C. Bower , P. Demorest

We performed a systematic analysis of all INTEGRAL observations from 2003 to 2009 of 14 Supergiant Fast X-ray Transients (SFXTs), implying a net exposure time of about 30Ms. For each source we obtained lightcurves and spectra (3-100keV),…

High Energy Astrophysical Phenomena · Physics 2015-05-19 L. Ducci , L. Sidoli , A. Paizis

We report the outbursts from a newly discovered X-ray transient in the Magellanic-type, SB(s)m galaxy NGC 55. The transient source, XMMU J001446.81-391123.48, was undetectable in the 2001 \xmm{} and 2004 \chandra{} observations, but…

High Energy Astrophysical Phenomena · Physics 2015-02-26 V. Jithesh , Zhongxiang Wang

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…

High Energy Astrophysical Phenomena · Physics 2016-02-03 L. Sidoli , A. Paizis , K. Postnov

The hard X-ray sensitivity and arcminute position accuracy of the recently launched International Gamma-Ray Laboratory (INTEGRAL) has lead to the (re-)discovery of a class of heavily absorbed hard X-ray sources lying in the Galactic plane.…

Astrophysics · Physics 2009-11-07 J. Rodriguez , J. A. Tomsick , L. Foschini , R. Walter , A. Goldwurm , S. Corbel , P. Kaaret

IGR J16493-4348 was one of the first new sources to be detected by the INTEGRAL gamma-ray telescope in the 18-100 keV energy band. Based upon spatial coincidence the source was originally associated with the free radio pulsar PSR…

Astrophysics · Physics 2009-11-13 A. B. Hill , A. J. Dean , R. Landi , V. A. McBride , A. De Rosa , A. J. Bird , A. Bazzano , V. Sguera

We report on the BeppoSAX/WFC observation of a strong type-I X-ray burst from the recently discovered transient source SAX J1810.8-2609. The observed event showed evidence of photospheric radius expansion due to super-Eddington burst…

We report the discovery of a fairly bright transient during observations with the Wide Field Cameras on board the BeppoSAX satellite in September 1996. It was detected at a peak intensity of 0.1 Crab (2 to 10 keV) and lasted between 6 and…

Astrophysics · Physics 2008-11-26 J. J. M. in 't Zand , J. Heise , J. M. Muller , A. Bazzano , M. Cocchi , L. Natalucci , P. Ubertini