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Related papers: MS 1603.6+2600: an Accretion Disc Corona source?

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We found diffuse hard X-ray sources, G11.0+0.0, G25.5+0.0, and G26.6-0.1 in the ASCA Galactic plane survey data. The X-ray spectra are featureless with no emission line, and are fitted with both models of a thin thermal plasma in…

Astrophysics · Physics 2009-11-07 Aya Bamba , Masaru Ueno , Katsuji Koyama , Shigeo Yamauchi

We present results of an observation with Suzaku of the dipping, periodic bursting low mass X-ray binary XB 1323-619. Using the energy band 0.8 - 70 keV, we show that the source spectrum is well-described as the emission of an extended…

High Energy Astrophysical Phenomena · Physics 2015-05-13 M. Balucinska-Church , T. Dotani , T. Hirotsu , M. J. Church

(Abridged) Spectral and time variability analysis of the region of the hard X-ray transient EXS 1737.9-2952 near the Galactic Centre (GC), using data from the Narrow Field Instruments of BeppoSAX is reported. The main results are the MECS…

Astrophysics · Physics 2007-05-23 J. Huovelin , J. Schultz , O. Vilhu , D. Hannikainen , P. Muhli , Ph. Durouchoux

We present temporal and spectral properties of a unique X-ray dip in GX 301-2 as seen with Rossi X-ray Timing Explorer in May 2010. The X-ray pulsation from the source gradually declined prior to the dip, disappears for one spin cycle…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Ersin Gogus , Ingo Kreykenbohm , Tomaso Belloni

We report the discovery of an eclipsing X-ray binary with a 3.62-hr period within 24" of the center of the dwarf starburst galaxy NGC 4214. The orbital period places interesting constraints on the nature of the binary, and allows for a few…

We present the results of a 63 ks {\it Chandra} observation of the "supernova impostor" SN 2010da four months after it was first observed on 25 May 2010. We detect an X-ray source at $\sim7\sigma$ confidence coincident with the optical…

High Energy Astrophysical Phenomena · Physics 2015-05-28 B. Binder , B. F. Williams , A. K. H. Kong , T. J. Gaetz , P. P. Plucinsky , J. J. Dalcanton , D. R. Weisz

The outbursts of low mass X-ray binaries are prolonged relative to those of dwarf nova cataclysmic variables as a consequence of X-ray irradiation of the disc. We show that the time-scale of the decay light curve and its luminosity at a…

Astrophysics · Physics 2008-11-26 Craig R. Powell , Carole A. Haswell , Maurizio Falanga

In this Paper we report on our analysis of three Chandra observations of the accretion-powered millisecond X-ray pulsar IGR J00291+5934 obtained during the late stages of the 2004 outburst. We also report the serendipitous detection of the…

We have obtained the first broad-band X-ray spectra of the nearby compact elliptical galaxy M32 by using the ASCA satellite. The extracted spectra and X-ray luminosity are consistent with the properties of the hard spectral component…

Astrophysics · Physics 2009-10-30 M. Loewenstein , K. Hayashida , T. Toneri , D. S. Davis

We report on the discovery of a transient X-ray pulsars, located in the Small Magellanic Cloud, with a pulse period of 292 s. A series of Chandra pointings fortuitously recorded in 2010 April-May the occurrence of a two-weeks-long outburst,…

High Energy Astrophysical Phenomena · Physics 2013-08-06 P. Esposito , G. L. Israel , L. Sidoli , G. A. Rodríguez Castillo , N. Masetti , P. D'Avanzo , S. Campana

The X-ray source 2XMM J123103.2+110648 was previously found to show pure thermal X-ray spectra and a ~3.8 hr periodicity in three XMM-Newton X-ray observations in 2003-2005, and the optical spectrum of the host galaxy suggested it as a type…

High Energy Astrophysical Phenomena · Physics 2017-04-12 Dacheng Lin , Olivier Godet , Luis C. Ho , Didier Barret , Natalie A. Webb , Jimmy A. Irwin

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…

We report the discovery of 0.59 s X-ray pulsations from the low-mass X-ray binary, 5.57 hr dipping and eclipsing ADC source 2A 1822-371. Pulse arrival time analysis indicates a circular orbit with e < 0.03 (95% confidence) and an asini for…

Astrophysics · Physics 2009-11-06 Peter G. Jonker , Michiel van der Klis

We present XMM-Newton observations of the eclipsing polar EP Dra which cover nearly 3 binary orbital cycles. The X-ray and UV data show evidence for a prominent dip before the eclipse which is due to the accretion stream obscuring the…

Astrophysics · Physics 2009-11-10 Gavin Ramsay , C. M. Bridge , Mark Cropper , K. O. Mason , F. A. Cordova , W. Priedhorsky

The Chandra Multiwavelength Plane (ChaMPlane) Survey aims to constrain the Galactic population of mainly accretion-powered, but also coronal, low-luminosity X-ray sources (Lx <~ 1e33 erg/s). To investigate the X-ray source content in the…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Maureen van den Berg , Kyle Penner , JaeSub Hong , Jonathan E. Grindlay , Ping Zhao , Silas Laycock , Mathieu Servillat

The transient X-ray binary pulsar A0535+262 was observed with Suzaku on 2005 September 14 when the source was in the declining phase of the August-September minor outburst. The ~103 s X-ray pulse profile was strongly energy dependent, a…

4U 1822-37 is a Low Mass X-ray Binary (LMXB) system with an Accretion Disk Corona. We have obtained 16 new mid-eclipse time measurements of this source during the last 13 years using X- ray observations made with the RXTE-PCA, RXTE-ASM,…

High Energy Astrophysical Phenomena · Physics 2010-07-13 Chetana Jain , Biswajit Paul , Anjan Dutta

We report the detection of six discrete, low-luminosity (Lx < 10^33 erg/s) X-ray sources, located within 12 arcsec of the center of the collapsed-core globular cluster M30 (NGC 7099), and a total of 13 sources within the half-mass radius,…

In this paper, we report on the available X-ray data collected by INTEGRAL, Swift, and XMM-Newton during the first outburst of the INTEGRAL transient IGR J17451-3022, discovered in 2014 August. The monitoring observations provided by the…

High Energy Astrophysical Phenomena · Physics 2016-04-13 E. Bozzo , P. Pjanka , P. Romano , A. Papitto , C. Ferrigno , S. Motta , A. A. Zdziarski , F. Pintore , T. Di Salvo , L. Burderi , D. Lazzati , G. Ponti , L. Pavan

Emission of two short hard X-ray bursts on 2009 June 5 disclosed the existence of a new soft gamma-ray repeater, now catalogued as SGR 0418+5729. After a few days, X-ray pulsations at a period of 9.1 s were discovered in its persistent…

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