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相关论文: X-ray outbursts from a new transient in NGC 55

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We present the spectral and temporal properties of 15 candidate transient X-ray sources detected in archival {\it XMM-Newton} and {\it Chandra} observations of the nearby Magellanic-type, SB(s)m galaxy NGC 55. On the basis of an X-ray color…

高能天体物理现象 · 物理学 2016-04-14 V. Jithesh , Zhongxiang Wang

We present an analysis of the X-ray properties of the Magellanic-type galaxy NGC 55 based on two contiguous XMM-Newton observations. We detect a total of 137 X-ray sources in the field of view, 42 of which are located within the optical…

天体物理学 · 物理学 2009-11-11 A-M. Stobbart , T. P. Roberts , R. S. Warwick

XMM-Newton EPIC observations have revealed a bright point-like X-ray source in the nearby Magellanic-type galaxy NGC 55. At the distance of NGC 55, the maximum observed X-ray luminosity of the source, designated as XMMU J001528.9-391319, is…

天体物理学 · 物理学 2009-11-10 A-M. Stobbart , T. P. Roberts , R. S. Warwick

We report the identification of seven transient X-ray sources in the nearby Magellanic-type galaxy NGC 4449 using the archival multi-epoch X-ray observations conducted with {\it Chandra}, {\it XMM-Newton} and {\it Swift} telescopes over…

高能天体物理现象 · 物理学 2017-02-09 V. Jithesh , Zhongxiang Wang

We present the results of X-ray observations of four bright transients sources detected in the July 2004 XMM-Newton observations of the central bulge of M31. Two X-ray sources, XMMU J004315.5+412440 and XMMU J004144.7+411110, were…

天体物理学 · 物理学 2008-11-26 Sergey Trudolyubov , William Priedhorsky , France Cordova

We report the discovery of a bright X-ray transient object, XMMU J174554.4-285456, observed in outburst with XMM-Newton on October 3, 2002,and located at 6.3' from SgrA*, the supermassive black hole at the Galactic center.This object…

天体物理学 · 物理学 2009-11-10 D. Porquet , N. Grosso , V. Burwitz , I. L. Andronov , B. Aschenbach , P. Predehl , R. S. Warwick

We study three transient X-ray sources, that were bright in the central region of M31 galaxy in the year 2000. Observations with Chandra and XMM-Newton allowed us for the first time in the history of X-ray astronomy, to build light curves…

天体物理学 · 物理学 2009-11-07 S. Trudolyubov , K. Borozdin , W. Priedhorsky

The transient X-ray source XMMU J004215.8+411924 within M31 was found to be in outburst again in the 2010 May 27 Chandra observation. We present results from our four Chandra and seven Swift observations that covered this outburst. X-ray…

高能天体物理现象 · 物理学 2015-05-20 R. Barnard , M. Garcia , S. Murray , N. Nooraee , W. Pietsch

During the third all-sky survey (eRASS3), eROSITA, the soft X-ray instrument aboard Spectrum-Roentgen-Gamma, detected a new hard X-ray transient, eRASSt J040515.6-745202, in the direction of the Magellanic Bridge. We arranged follow-up…

The purpose of this study is to find transient X-ray sources in M31, and to investigate and classify their nature. Three X-ray transients were observed with Swift. For each of the three X-ray transients we use the Swift X-ray and optical…

天体物理学 · 物理学 2009-11-13 R. Voss , W. Pietsch , F. Haberl , H. Stiele , J. Greiner , G. Sala , D. H. Hartmann , D. Hatzidimitriou

We report the discovery of a bright X-ray transient, CXOU J132527.6-430023, in the nearby early-type galaxy NGC 5128. The source was first detected over the course of five Chandra observations in 2007, reaching an unabsorbed outburst…

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

I report on the discovery and analysis of the first transient X-ray pulsar detected in the Local Group galaxy M33. The 2010 July-August deep XMM-Newton observations of M33 fields revealed a new bright X-ray source XMMU J013359.5+303634…

高能天体物理现象 · 物理学 2017-01-10 Sergey Trudolyubov

We present the results from RXTE observations of a new X-ray transient, GRS 1737-31, near the Galactic center during an outburst. Over a span of two weeks, the source was seen to vary significantly on time scales down to a few seconds. The…

天体物理学 · 物理学 2009-10-30 Wei Cui , W. A. Heindl , J. H. Swank , D. M. Smith , E. H. Morgan , R~. Remillard , F. E. Marshall

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 on the results of a four-year long X-ray monitoring campaign of the central 1.2 square degrees of our Galaxy, performed with Chandra and XMM-Newton between 2005 and 2008. Our study focuses on the properties of transient X-ray…

高能天体物理现象 · 物理学 2015-06-04 N. Degenaar , R. Wijnands , E. M. Cackett , J. Homan , J. J. M. in 't Zand , E. Kuulkers , T. J. Maccarone , M. van der Klis

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…

高能天体物理现象 · 物理学 2015-05-30 Joseph R. Callingham , Sean A. Farrell , Bryan M. Gaensler , Geraint F. Lewis , Matthew J. Middleton

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 present the results of a study of the variability of X-ray sources in the central 30' of the nearby Andromeda Galaxy (M31) based on XMM Performance Verification observations. Two observations of this field, with a total exposure time of…

We report on the serendipitous discovery of a new transient in NGC 5907, at a peak luminosity of 6.4x10^{39} erg/s. The source was undetected in previous 2012 Chandra observations with a 3 sigma upper limit on the luminosity of 1.5x10^{38}…

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