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相关论文: An Unusual X-ray Burst from the Globular Cluster M…

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The Low Mass X-ray Binary (LMXB) X1822-330 in NGC 6652 is one of 12 bright, or transient, X-ray sources to have been discovered in Globular Clusters. We report on a serendipitous ASCA observation of this Globular Cluster LMXB, during which…

天体物理学 · 物理学 2009-10-31 Koji Mukai , Alan P. Smale

During a BeppoSAX observation of the X-ray burst source X1732-304 located in the globular cluster Terzan 1 in 1999 April, the source was detected in an anomalously low-state with an X-ray luminosity of 1.4 x 10^33 erg/s$, about 300 times…

天体物理学 · 物理学 2007-05-23 M. Guainazzi , A. N. Parmar , T. Oosterbroek

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

During a 50 ks monitoring observation of the Galactic bulge performed in September 1999 by the Wide Field Cameras on board the BeppoSAX satellite, an X-ray burst was detected from a sky position ~3 degrees off the Galactic centre. No…

天体物理学 · 物理学 2009-11-07 M. Cocchi , A. Bazzano , L. Natalucci , P. Ubertini , J. Heise , E. Kuulkers , R. Cornelisse , J. J. M. in 't Zand

Our 5 ks Chandra ACIS-S observation of the globular cluster NGC 6652 detected 7 X-ray sources, 3 of which are previously unidentified. This cluster hosts a well-known bright low-mass X-ray binary, source A (or XB 1832-330). Source B shows…

高能天体物理现象 · 物理学 2015-05-28 G. Coomber , C. O. Heinke , H. N. Cohn , P. M. Lugger , J. E. Grindlay

We report the discovery of several optical burst-like events from the low-mass X-ray binary MS1603.6+2600 (UW CrB). The events last for a few tens of seconds, exhibit a very fast rise and slow decay, and involve optical brightening of a…

天体物理学 · 物理学 2009-11-10 R. I. Hynes , E. L. Robinson , E. Jeffery

We report the serendipitous detection with the Rossi X-ray Timing Explorer of a long and peculiar X-ray burst whose localization is consistent with one known X-ray burster (GRS 1747-312) and which occurred when that source was otherwise…

天体物理学 · 物理学 2009-11-10 J. J. M. in 't Zand , T. E. Strohmayer , C. B. Markwardt , J. Swank

Two type I X-ray bursts were detected from a position consistent with the transient X-ray source in NGC 6652 with the Wide Field Camera of the BeppoSAX satellite, strongly suggesting that this transient is a neutron star. Our detection…

天体物理学 · 物理学 2008-11-26 J. J. M. in 't Zand , F. Verbunt , J. Heise , J. M. Muller , A. Bazzano , M. Cocchi , L. Natalucci , P. Ubertini

INTEGRAL detected on August 31, 2004, an unusual thermonuclear X-ray burst from the low-mass X-ray binary GX 3+1. Its duration was 30 min, which is between the normal burst durations for this source (<~10 s) and the superburst observed in…

Ultraluminous X-ray bursts (hereafter ULXBs) are ultraluminous X-ray flares with a fast rise ($\sim$ one minute) and a slow decay ($\sim$ an hour), which are commonly observed in extragalactic globular clusters. Most ULXBs are observational…

高能天体物理现象 · 物理学 2022-09-21 Hao-Yan Chen , Wei-Min Gu , Jin-Bo Fu , Shan-Shan Weng , Junfeng Wang , Mouyuan Sun

There have been several recent claims of black hole binaries in globular clusters. I show that these candidate systems could instead be ultracompact X-ray binaries (UCXBs) in which a neutron star accretes from a white dwarf. They would…

星系天体物理 · 物理学 2015-05-27 Andrew King

We report the discovery of millisecond oscillations in an X-ray burst from the X-ray transient SAX J1748.9-2021 in the globular cluster NGC 6440. Oscillations at a frequency of 409.7 +/- 0.3 Hz were present in one of nine X-ray bursts…

天体物理学 · 物理学 2009-11-07 P. Kaaret , J. J. M. in 't Zand , J. Heise , J. A. Tomsick

We report the finding of an unusual, weak precursor to a thermonuclear X-ray burst from the accreting millisecond pulsar SAX J1808.4-3658. The burst in question was observed on Oct. 19, 2002 with the Rossi X-Ray Timing Explorer (RXTE)…

天体物理学 · 物理学 2008-11-26 Sudip Bhattacharyya , Tod E. Strohmayer

We report an observation by the Chandra X-ray Observatory of 4U2127+119, the X-ray source identified with the globular cluster M15. The Chandra observation reveals that 4U2127+119 is in fact two bright sources, separated by 2.7". One source…

天体物理学 · 物理学 2009-11-07 Nicholas E. White , Lorella Angelini

The prototypical post-core-collapse globular cluster M15 provides an ideal environment for the formation of exotic binaries, it being already known to contain a luminous LMXB (X2127+119, optically identified with the 17.1 hour eclipsing…

天体物理学 · 物理学 2009-11-07 P. A. Charles , W. I. Clarkson , L. van Zyl

The neutron star low-mass X-ray binary GRS 1741.9-2853 is a known type-I burster of the Galactic Center. It is transient, faint, and located in a very crowded region, only 10 arcmin from the supermassive black hole Sgr A*. Therefore, its…

高能天体物理现象 · 物理学 2015-05-13 G. Trap , M. Falanga , A. Goldwurm , E. Bozzo , R. Terrier , P. Ferrando , D. Porquet , N. Grosso , M. Sakano

We observed the nearby, low-density globular cluster M71 (NGC 6838) with the Chandra X-ray Observatory to study its faint X-ray populations. Five X-ray sources were found inside the cluster core radius, including the known eclipsing binary…

For the first time X-ray bursts have been detected from a sky position consistent with the one of GRS 1741.9-2853, a GRANAT transient source located only ~10' from the Galactic Centre. A total of 3 bursts have been observed by the Wide…

天体物理学 · 物理学 2007-05-23 M. Cocchi , A. Bazzano , L. Natalucci , P. Ubertini , J. Heise , J. M. Muller , J. J. M. in 't Zand

The prototypical accretion-powered millisecond pulsar SAX J1808.4-3658 was observed simultaneously with Chandra-LETGS and RXTE-PCA near the peak of a transient outburst in November 2011. A single thermonuclear (type-I) burst was detected,…

We report on a thermonuclear (type-I) X-ray burst that was detected from the neutron star low-mass X-ray binary SAX J1810.8-2609 in 2007 with Swift. This event was longer (~20 min) and more energetic (a radiated energy of Eb~6.5E39 erg)…

高能天体物理现象 · 物理学 2015-06-11 N. Degenaar , R. Wijnands
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