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Related papers: The SMC X-ray transient XTE J0111.2-7317 : a Be/X-…

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We report on the discovery and confirmation of the optical counterparts of the two transient X-ray pulsars, RXJ0052.1-7319 and XTEJ0111.2-7317. In the narrow (~3" radius) X-ray error circle of RXJ0052.1-7319 we found a V=14.6 (B-V=0.1)…

We report on two optical candidates for the counterpart to an X-ray source in the SMC, 1WGA J0053.8-7226, identified as a serendipitous X-ray source from the ROSAT PSPC archive, and also observed by the Einstein IPC. Its X-ray properties,…

We report observations which confirm the identities of the optical counterpart to the transient sources RX J0544.1-7100 and RX J0520.5-6932. The counterparts are suggested to be a B-type stars. Optical data from the observations carried out…

Astrophysics · Physics 2009-11-06 M. J. Coe , I. Negueruela , D. A. H. Buckley , N. J. Haigh , S. G. T. Laycock

We present optical spectroscopy and optical and infrared photometry of the counterpart to the transient X-ray source KS 1947+300. The counterpart is shown to be a moderately reddened V=14.2 early-type Be star located in an area of low…

A new x-ray transient, designated XTE J1739-302, was discovered with the Proportional Counter Array (PCA) on the Rossi X-ray Timing Explorer (RXTE) in data from 12 August 1997. Although it was the brightest source in the Galactic Center…

We present the results of our search for optical counterparts to high-mass X-ray transient sources discovered by various X-ray missions. We obtained CCD images of the X-ray fields through BVR and Halpha filters in order to identify…

Astrophysics · Physics 2009-11-11 P. Reig , I. Negueruela , G. Papamastorakis , A. Manousakis , T. Kougentakis

We continue to study the fast X-ray transient XTE J1901+014 discovered in 2002 by the RXTE observatory, whose nature has not yet been established. Based on the XMM-Newton observations of the source in 2006, we have obtained its energy…

Astrophysics · Physics 2009-11-13 D. I. Karasev , A. A. Lutovinov , R. A. Burenin

We report on the discovery of the optical/IR counterpart of the 15.8s transient X-ray pulsar XTE J1946+274. We re-analysed archival BeppoSAX observations of XTE J1946+274, obtaining a new refined position (a circle with 22" radius at 90%…

We identify the probable optical counterpart of the SMC supersoft source, RX~J0059.2-7138, with a $\sim$~14th magnitude star lying within the X-ray error circle. We present high resolution optical spectroscopy, which reveals strong HI…

Astrophysics · Physics 2016-06-08 K. A. Southwell , P. A. Charles

The observed characteristics of the nebulosity surrounding the SMC High Mass X-ray Binary XTE J0111.2-7317 are examined in the context of three possible nebular types: SNR, bowshock and HII region. Observational evidence is presented which…

Astrophysics · Physics 2009-11-07 M. J. Coe , N. J. Haigh , C. A. Wilson , I. Negueruela

We report the discovery of a new X-ray pulsar, XTE J1810-197. The source was serendipitously discovered on 2003 July 15 by the Rossi X-ray Timing Explorer (RXTE) while observing the soft gamma repeater SGR 1806-20. The pulsar has a 5.54 s…

The X-ray transient MXB 0656-072 is a poorly studied member of high-mass X-ray binaries. Based on the transient nature of the X-ray emission, the detection of pulsations, and the early-type companion, it has been classified as a Be X-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-05 E. Nespoli , P. Reig , A. Zezas

Recent observations of the Small Magellanic Cloud (SMC) with Einstein Probe (EP) revealed a new transient X-ray source, most likely identified as Be/X-ray binary. To characterise the X-ray properties of EP J005146.9-730930 and in particular…

High Energy Astrophysical Phenomena · Physics 2025-07-24 F. Haberl , Y. Xu , C. Maitra , G. Vasilopoulos , W. Zhang , W. Yuan , C. Jin , H. N. Yang , L. Ducci , D. M. Kaltenbrunner , P. Maggi , A. Rau

We have discovered with the Wide Field Cameras on board BeppoSAX the weak transient X-ray source SAXJ2239.3+6116 whose position coincides with that of 4U2238+60/3A2237+608 and is close to that of the fast transient AT2238+60 and the…

We report the discovery of an X-ray transient, observed in outburst with XMM-Newton on March 20, 2003, and with position 18h12m27.8s, -18 12 34 (J2000, approximate positional error 2"). No known source is present at this position and the…

Astrophysics · Physics 2009-11-11 Edward M. Cackett , Rudy Wijnands , Ron Remillard

Swift J004929.5-733107 is an X-ray source in the Small Magellanic Cloud (SMC) that has been reported several times, but the optical counterpart has been unclear due to source confusion in a crowded region of the SMC. Previous works proposed…

High Energy Astrophysical Phenomena · Physics 2021-04-21 M. J. Coe , J. A. Kennea , P. A. Evans , L. J. Townsend , A. Udalski , I. M. Monageng , D. A. H. Buckley

We report the discovery of Type I (thermonuclear) X-ray bursts from the transient source XMMU J181227.8-181234 = XTE J1812-182. We found 7 X-ray bursts in Rossi X-ray Timing Explorer observations during the 2008 outburst, confirming the…

High Energy Astrophysical Phenomena · Physics 2019-05-01 A. J. Goodwin , D. K. Galloway , J. J. M. in 't Zand , E. Kuulkers , A. Bilous , L. Keek

The weak X-ray transient XTE J1739-302, characterized by extremely short outbursts, has recently been identified with a reddened star. Here we present spectroscopy and photometry of the counterpart, identifying it as a O8Iab(f) supergiant…

We present detailed analysis of the transient X-ray source 2XMMi J003833.3+402133 detected by XMM-Newton in January 2008 during a survey of M 31. The X-ray spectrum is well fitted by either a steep power law plus a blackbody model or a…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Joseph R. Callingham , Sean A. Farrell , Bryan M. Gaensler , Geraint F. Lewis , Matthew J. Middleton

Details of simultaneous photometric and spectroscopic observations of the optical counterpart of the `supersoft' X-ray source 1E 0035.4-7230 (SMC 13) are presented. Although the spectrum is dominated by emission lines of He II, the Balmer…

Astrophysics · Physics 2007-05-23 David Crampton , J. B. Hutchings , A. P. Cowley , P. C. Schmidtke
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