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

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The newly discovered 11 Hz accreting pulsar, IGR J17480-2446, located in the globular cluster Terzan 5, has shown several bursts with a recurrence time as short as few minutes. The source shows the shortest recurrence time ever observed…

高能天体物理现象 · 物理学 2015-05-27 S. Motta , A. D'Aì , A. Papitto , A. Riggio , T. Di Salvo , L. Burderi , T. Belloni L. Stella , R. Iaria

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…

天体物理学 · 物理学 2009-02-18 M. P. Muno , J. R. Lu , F. K. Baganoff , W. N. Brandt , G. P. Garmire , A. M. Ghez , S. D. Hornstein , M. R. Morris

We present a study of two X-ray bursters in the Galactic Center field with the ART-P telescope onboard GRANAT. During 1990-1992 approximately 100 X-ray bursts were detected from the Galactic Center field and most of them were identified…

天体物理学 · 物理学 2007-05-23 A. A. Lutovinov , S. A. Grebenev , M. N. Pavlinsky , R. A. Sunyaev

The discovery of a type I X-ray burst from the faint unidentified transient source IGR J17445-2747 in the Galactic bulge by the JEM-X telescope onboard the INTEGRAL observatory is reported. Type I bursts are believed to be associated with…

高能天体物理现象 · 物理学 2017-09-11 I. A. Mereminskiy , S. A. Grebenev , R. A. Sunyaev

Two short (<2 s) g-ray bursts (GRBs) have recently been localized and fading afterglow counterparts detected. The combination of these two results left unclear the nature of the host galaxies of the bursts, because one was a star-forming…

We report for the first time on the rapid X-ray variability of the galactic bulge source and X-ray burster SLX 1735-269. The power spectrum as observed with the Rossi X-ray Timing Explorer is characterized by a strong band-limited noise…

天体物理学 · 物理学 2007-05-23 Rudy Wijnands , Michiel van der Klis

We present a study of weak, thermonuclear X-ray bursts from the accreting millisecond X-ray pulsar SAX J1808.4-3658. We focus on a burst observed with the Neutron Star Interior Composition Explorer on 2019 August 9, and describe a similar…

高能天体物理现象 · 物理学 2023-05-26 Sierra Casten , Tod Strohmayer , Peter Bult

Quasi-periodic oscillations and X-ray spectroscopy are powerful probes of black hole masses and accretion disks, and here we apply these diagnostics to an ultraluminous X-ray source (ULX) in the spiral galaxy NGC628 (M74). This object was…

Type-I X-ray bursts are thermonuclear explosions occurring in the surface layers of accreting neutron stars. These events are powerful probes of the physics of neutron stars and their surrounding accretion flow. We analyze a very energetic…

高能天体物理现象 · 物理学 2015-06-12 N. Degenaar , J. M. Miller , R. Wijnands , D. Altamirano , A. C. Fabian

We report on our serendipitous discovery with the XMM-Newton Observatory of a luminous X-ray emitting cluster of galaxies that is located behind the Andromeda galaxy (M31). X-ray emission from the cluster was detected previously by ROSAT,…

天体物理学 · 物理学 2009-11-10 Oleg V. Kotov , Sergey Trudolyubov , W. Thomas Vestrand

Fast radio bursts are bright, millisecond-scale radio flashes of yet unknown physical origin. Recently, their extragalactic nature has been demonstrated and an increasing number of the sources have been found to repeat. Young, highly…

高能天体物理现象 · 物理学 2021-04-21 A. Ridnaia , D. Svinkin , D. Frederiks , A. Bykov , S. Popov , R. Aptekar , S. Golenetskii , A. Lysenko , A. Tsvetkova , M. Ulanov , T. Cline

We perform time-resolved spectroscopy of all the type I bursts from the Rapid Burster (MXB 1730-335) detected with the Rossi X-ray Timing Explorer. Type I bursts are detected at high accretion rates, up to \sim 45% of the Eddington…

高能天体物理现象 · 物理学 2013-03-14 T. Bagnoli , J. J. M. in 't Zand , D. K. Galloway , A. L. Watts

I present an observational review of the five currently known accretion-driven millisecond X-ray pulsars. A prominent place in this review is given to SAX J1808.4-3658; it was the first such system discovered and currently four outbursts…

天体物理学 · 物理学 2009-11-10 Rudy Wijnands

We report the discovery of a flaring X-ray source in the globular cluster NGC 6540, obtained during the EXTraS project devoted to a systematic search for variability in archival data of the XMM-Newton satellite. The source had a quiescent…

The unresolved X-ray emission in the cores of 10 globular clusters hosting millisecond pulsars is investigated. Subtraction of the known resolved point sources leads to detectable levels of unresolved emission in the core region of M28, NGC…

高能天体物理现象 · 物理学 2009-07-22 C. Y. Hui , K. S. Cheng , Ronald E. Taam

We searched for X-ray bursts in XMM-Newton archival data of X-ray sources in M 31 globular clusters (GCs) and GC candidates. We detected two bursts simultaneously in EPIC pn and MOS detectors and some more candidates in EPIC pn. The energy…

天体物理学 · 物理学 2009-11-10 W. Pietsch , F. Haberl

We report the discovery of an X-ray source coincident with the nuclear star cluster at the dynamical center of the nearby late-type spiral galaxy NGC 2403. The X-ray luminosity of this source varies from below detection levels, ~1e35 erg/s…

天体物理学 · 物理学 2011-02-11 Mihoko Yukita , Douglas A. Swartz , Roberto Soria , Allyn F. Tennant

We report the discovery of the second accreting millisecond X-ray pulsar (AMXP) in the globular cluster NGC 6440. Pulsations with a frequency of 205.89 Hz were detected with the Rossi X-Ray Timing Explorer on August 30th, October 1st and…

高能天体物理现象 · 物理学 2011-02-11 D. Altamirano , A. Patruno , C. Heinke , C. Markwardt , T. Strohmayer , M. Linares , R. Wijnands , M. van der Klis , J. Swank

We have conducted Chandra observations of ~2560 square arcmin (~131 kpc^2) of of M31, and find that the most luminous X-ray sources in our fields are in globular clusters (GCs). Of the 28 GC X-ray sources in our fields, 17 are newly…

天体物理学 · 物理学 2016-08-30 R. Di Stefano , A. K. H. Kong , M. R. Garcia , P. Barmby , J. Greiner , S. S. Murray , F. A. Primini

A previously undetected X-ray source (L_X<10**36 erg/s) in the strongly star-forming galaxy M83 entered an ultraluminous state between August 2009 and December 2010. It was first seen with Chandra on 23 December 2010 at L_X ~ 4 10**39…