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We have found an optical/X-ray counterpart candidate for the bright, but presently unidentified, Fermi source 2FGL J1311.7-3429. This counterpart undergoes large amplitude quasi-sinusoidal optical modulation with a 1.56h (5626s) period. The…

高能天体物理现象 · 物理学 2015-06-05 Roger W. Romani

We report on the discovery of coherent pulsations at a period of 2.9 ms from the X-ray transient MAXI J0911-655 in the globular cluster NGC 2808. We observed X-ray pulsations at a frequency of $\sim339.97$ Hz in three different observations…

高能天体物理现象 · 物理学 2017-02-01 A. Sanna , A. Papitto , L. Burderi , E. Bozzo , A. Riggio , T. Di Salvo , C. Ferrigno , N. Rea , R. Iaria

We report on X-ray observations made with the Rossi X-ray Timing Explorer of the black hole candidate (BHC) transient XTE J1650-500 at the end of its first, and currently only, outburst. By monitoring the source at low luminosities over…

天体物理学 · 物理学 2008-11-26 John A. Tomsick , Emrah Kalemci , Stephane Corbel , Philip Kaaret

An unidentified $\gamma$-ray source 4FGL J1838.2+3223 has been proposed as a pulsar candidate. We present optical time-series multi-band photometry of its likely optical companion obtained with the 2.1-m telescope of Observatorio…

高能天体物理现象 · 物理学 2023-11-20 D. A. Zyuzin , A. Yu. Kirichenko , A. V. Karpova , Yu. A. Shibanov , S. V. Zharikov , M. R. Gilfanov , C. Perez Tórtola

We present high time-resolution multicolour optical observations of the quiescent X-ray transients GRS1124-684 (=GU Mus) and Cen X-4 (=V822 Cen) obtained with ULTRACAM. Superimposed on the secondary stars' ellipsoidal modulation in both…

太阳与恒星天体物理 · 物理学 2015-05-14 T. Shahbaz , V. S. Dhillon , T. R. Marsh , J. Casares , C. Zurita , P. A. Charles

The recent discovery of a milli-second radio pulsar experiencing an accretion outburst similar to those seen in low mass X-ray binaries, has opened up a new opportunity to investigate the evolutionary link between these two different…

高能天体物理现象 · 物理学 2015-06-22 N. Degenaar , R. Wijnands , M. T. Reynolds , J. M. Miller , D. Altamirano , J. Kennea , N. Gehrels , D. Haggard , G. Ponti

We report the discovery of the X-ray transient SAX J2103.5+4545 which was active from February to September 1997. The observed peak intensity of 20 mCrab (2 to 25 keV) occurred on April 11. An analysis of data obtained around the time of…

天体物理学 · 物理学 2007-05-23 F. Hulleman , J. J. M. in 't Zand , J. Heise

We report an X-ray flare from 3XMM J014528.9+610729, serendipitously detected during the observation of the open star cluster NGC 663. The colour-colour space technique using optical and infrared data reveals the X-ray source as a candidate…

高能天体物理现象 · 物理学 2014-09-16 Himali Bhatt , Subir Bhattacharyya , Nilay Bhatt , J. C. Pandey

After nearly a decade in quiescence, the accreting millisecond pulsar IGR J17511$-$3057 displayed a new outburst on 2025 February 11, its third since discovery, following previous activity in 2009 and 2015. We report on an XMM-Newton Target…

IGR J17511-3057 is the second X-ray transient accreting millisecond pulsar discovered by INTEGRAL. It was in outburst for about a month from September 13, 2009. The broad-band average spectrum is well described by thermal Comptonization…

高能天体物理现象 · 物理学 2011-07-18 M. Falanga , L. Kuiper , J. Poutanen , D. K. Galloway , E. W. Bonning , E. Bozzo , A. Goldwurm , W. Hermsen , L. Stella

We report on the results of the ASCA and ROSAT observations on RX J0059.2-7138, a transient X-ray pulsar in the Small Magellanic Cloud. The barycentric pulse period has been precisely determined to be 2.763221 +- 0.000004 s. The pulse shape…

天体物理学 · 物理学 2015-06-24 Makoto Kohno , Jun Yokogawa , Katsuji Koyama

We report on observations of the unusual neutron-star binary system FIRST J102347.6+003841 carried out using the XMM-Newton satellite. This system consists of a radio millisecond pulsar in an 0.198-day orbit with a ~0.2 solar-mass…

We present X-ray observations of the "redback" eclipsing radio millisecond pulsar and candidate radio pulsar/X-ray binary transition object PSR J1723-2837. The X-ray emission from the system is predominantly non-thermal and exhibits…

高能天体物理现象 · 物理学 2015-06-17 Slavko Bogdanov , Paolo Esposito , Fronefield Crawford , Andrea Possenti , Maura A. McLaughlin , Paulo Freire

IGR J17591$-$2342 is a new accreting millisecond X-ray pulsar (AMXP) that was recently discovered in outburst in 2018. Early observations revealed that the source's radio emission is brighter than that of any other known neutron star…

In order to probe the activity of the inner disk flow and its effect on the neutron star surface emissions, we carried out the timing analysis of the Rossi X-Ray Timing Explorer (RXTE) observations of the millisecond X-ray pulsar XTE…

天体物理学 · 物理学 2008-11-26 Fan Zhang , J. L. Qu , C. M. Zhang , W. Chen , T. P. Li

XSS J12270-4859 (henceforth J12270) is the first low-mass X-ray binary to exhibit a transition, taking place at the end of 2012, from an X-ray active state to a radio pulsar state. The X-ray emission based on archival XMM-Newton…

高能天体物理现象 · 物理学 2020-03-04 Miraval Zanon , A. , Campana , S. , Ridolfi , A. , D'Avanzo , P. , Ambrosino F

We have discovered four X-ray bursts, recorded with the Rossi X-ray Timing Explorer Proportional Counter Array between 2003 September and 2004 April, that we show to originate from the transient magnetar candidate XTE J1810-197. The burst…

We present the study of multi-wavelength observations of an unidentified Fermi Large Area Telescope (LAT) source, 4FGL J1910.7-5320, a new candidate redback millisecond pulsar binary. In the 4FGL 95% error region of 4FGL J1910.7-5320, we…

We present a multifrequency study of the transient $\gamma$-ray source 4FGL J1544.3-0649, a blazar that exhibited a remarkable behaviour raising from the state of an anonymous mid-intensity radio source, never detected at high energies, to…

高能天体物理现象 · 物理学 2021-01-13 N. Sahakyan , P. Giommi

We report on optical and X-ray observations of the accretion powered ms pulsar IGR J00291+5934 in quiescence. Time resolved I-band photometry has been obtained with the 4.2 m William Herschel Telescope, while a 3 ks Chandra observation…

天体物理学 · 物理学 2008-02-19 P. G. Jonker , M. A. P. Torres , D. Steeghs