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相关论文: X-Ray Eclipse Time Delays in 4U2129+47

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The ultracompact low-mass X-ray binary 4U 0513-40 in the globular cluster NGC1851 exhibits large amplitude X-ray flux variations with spectral changes from low/hard to high/soft states which have not been reported previously in other…

高能天体物理现象 · 物理学 2015-05-27 M. Fiocchi , A. Bazzano , L. Natalucci , R. Landi , P. Ubertini

The ultracompact X-ray binary 4U 1820-30 is well known for its ~170-d superorbital modulation in X-ray flux and spectrum, and the exclusiveness of bursting behavior to the low hard 'island' state. In May-June 2009, there was an…

高能天体物理现象 · 物理学 2015-06-11 J. J. M. in 't Zand , J. Homan , L. Keek , D. M. Palmer

We present a detailed optical study of the ultra-compact X-ray binary 4U0614+091. We have used 63 hrs of time-resolved optical photometry taken with three different telescopes (IAC80, NOT and SPM) to search for optical modulations. The…

天体物理学 · 物理学 2009-11-13 T. Shahbaz , C. A. Watson , C. Zurita , E. Villaver , H. Hernandez-Peralta

The accretion flow / jet correlation in neutron star (NS) low-mass X-ray binaries (LMXBs) is far less understood when compared to black hole (BH) LMXBs. In this paper we will present the results of a dense multi-wavelength observational…

The Galactic black hole (BH) X-ray binary 4U 1630-47 went into a new outburst in 2021 after $\sim$ 600 days from its 2020 outburst. We perform a detailed analysis of quasi-periodic oscillations and spectral evolutions during its 2021…

高能天体物理现象 · 物理学 2025-06-25 Jiashi Chen , Wei Wang

We performed a search for eclipsing and dipping sources in the archive of the EXTraS project - a systematic characterization of the temporal behaviour of XMM-Newton point sources. We discovered dips in the X-ray light curve of 3XMM…

高能天体物理现象 · 物理学 2017-12-27 M. Marelli , A. Tiengo , A. De Luca , D. Salvetti , L. Saronni , L. Sidoli , A. Paizis , R. Salvaterra , A. Belfiore , G. Israel , F. Haberl , D. D'Agostino

We report the results from an X-ray and near-infrared observation of the Galactic black hole binary 4U 1630--47 in the very high state, performed with {\it Suzaku} and IRSF around the peak of the 2012 September-October outburst. The X-ray…

We report the first statistically significant detection of X-ray polarization from the high-mass X-ray binary (HMXB) 4U 1700-377, observed using the Imaging X-ray Polarimetry Explorer (IXPE). A polarization degree exceeding 10% was detected…

We report on the X-ray spectral and timing behavior of the recurrent X-ray transient 4U 1630-47 for 51 RXTE observations made during the decay of its 1998 outburst. The observations began when the source was still relatively bright, and,…

天体物理学 · 物理学 2009-10-31 John A. Tomsick , Philip Kaaret

We report the superburst from 4U 1820--30 in 2021 observed by the Monitor of All-sky X-ray Image and Neutron star Interior Composition Explorer (NICER). During the tail of the superburst, we found that the NICER light curve unexpectedly…

高能天体物理现象 · 物理学 2025-03-14 Zhijiao Peng , Zhaosheng Li , Yuanyue Pan , Tao Fu , Wenhui Yu , Yupeng Chen , Shu Zhang , Maurizio Falanga , Shuang-Nan Zhang

[abridged] The LMXB 4U 0614+091 is a source of sporadic thermonuclear (type I) X-ray bursts. We find bursts with a wide variety of characteristics in serendipitous wide-field X-ray observations by EURECA/WATCH, RXTE/ASM, BeppoSAX/WFC,…

A probable binary period has been detected in the optical counterpart to the X-ray source CXOU J005455.6-724510 = RX J0054.9-7245 = AXJ0054.8-7244 = SXP504 in the Small Magellanic Cloud. This source was detected by Chandra on 04 Jul 2002…

Ultra-luminous X-Ray Objects are off-nucleus point sources with $L_X=10^{39}$-$10^{41}$ erg/s but the nature of such systems are largely unidentified. Here we report a 2.1 hour period observed in a Chandra ACIS observation for ULX M51 X-7,…

天体物理学 · 物理学 2009-11-07 Ji-Feng Liu , Joel N. Bregman , Jimmy Irwin , Patrick Seitzer

[abridged] Three years of optical monitoring of the low-mass X-ray binary (LMXB) 4U 1957+11 is presented. The source was observed in V, R and i-bands using the Faulkes Telescopes North and South. The light curve is dominated by long-term…

高能天体物理现象 · 物理学 2015-05-14 D. M. Russell , F. Lewis , P. Roche , J. S. Clark , E. Breedt , R. P. Fender

We present the results of an analysis of data covering 1.5 years of the dwarf nova V447 Lyr. We detect eclipses of the accretion disk by the mass donating secondary star every 3.74 hrs which is the binary orbital period. V447 Lyr is…

太阳与恒星天体物理 · 物理学 2015-06-05 Gavin Ramsay , John K. Cannizzo , Steve B. Howell , Matt A. Wood , Martin Still , Thomas Barclay , Alan Smale

4U 1630-47 is a black-hole X-ray transient with one of the shortest recurrence times. Despite its regular outburst behaviour little is known about this source. Only recently has attention to this system increased. I discuss there the basic…

天体物理学 · 物理学 2009-10-30 Erik Kuulkers

A pointed observation of the low-luminosity galactic source 4U 2206+54 was carried out in November 1998 with BeppoSAX. The light curve of 4U 2206+54 shows erratic variability on a timescale of about 1 hour; neither hardness variations nor…

天体物理学 · 物理学 2009-11-10 N. Masetti , D. Dal Fiume , L. Amati , S. Del Sordo , F. Frontera , M. Orlandini , E. Palazzi

We present a study of the distribution of asymptotic burst oscillation periods for a sample of 26 bursts from 4U 1636-53 observed with the Rossi X-ray Timing Explorer (RXTE). The burst sample includes both archival and proprietary data and…

天体物理学 · 物理学 2009-11-07 A. B. Giles , K. M. Hill , T. E. Strohmayer , N. Cummings

We have observed the eclipsing low-mass X-ray binary MS1603.6+2600 with Chandra for 7 ksec. The X-ray spectrum is well fit with a single absorbed powerlaw with an index of ~2. We find a clear sinusoidal modulation in the X-ray lightcurve…

天体物理学 · 物理学 2009-11-10 P. G. Jonker , M. van der Klis , C. Kouveliotou , M. Mendez , W. H. G. Lewin , T. Belloni

We report on XMM-Newton observations of the black hole X-ray binary 4U 1630-47 during its 2012-2013 outburst. The first five observations monitor the source as its luminosity increases across the high-soft state of accretion. In the sixth…

高能天体物理现象 · 物理学 2014-11-19 M. Díaz Trigo , S. Migliari , J. C. A. Miller-Jones , M. Guainazzi