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Related papers: Rapid Bursts From GRS 1915+105 with RXTE

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Low Mass X-Ray Binaries (LMXBs) are systems in which a compact object accretes from a binary companion star via an accretion disk. The X-ray properties of LMXBs show strong variability over timescales ranging from milliseconds to decades,…

High Energy Astrophysical Phenomena · Physics 2019-03-19 James Matthew Christopher Court

The origin of the large-amplitude, quasi-periodic X-ray flux variations in several classes of the Galactic microquasar GRS~1915+105 remains unresolved. We address this issue through flux-resolved, broadband (0.8-20 keV) spectral modelling…

High Energy Astrophysical Phenomena · Physics 2026-02-13 Shree Suman , Shuvajit Khatua , Vishal Jadoliya , Prathamesh Narayan Gupta , Mayukh Pahari

We report the discovery of an exceptionally short burst recurrence time in the well-known clocked burster GS 1826$-$238, observed with the CubeSat X-ray observatory NinjaSat. In 2025 May, GS 1826$-$238 underwent a soft-to-hard state…

Thermonuclear X-ray bursts from accreting neutron stars power brief but strong irradiation of their surroundings, providing a unique way to study accretion physics. We analyze MAXI/GSC and Swift/XRT spectra of a day-long flash observed from…

High Energy Astrophysical Phenomena · Physics 2017-02-22 L. Keek , W. Iwakiri , M. Serino , D. R. Ballantyne , J. J. M. in 't Zand , T. E. Strohmayer

We present 5-GHz MERLIN radio images of the microquasar GRS 1915+105 during two separate outbursts in 2001 March and 2001 July, following the evolution of the jet components as they move outwards from the core of the system. Proper motions…

We present evidence that ~ 30 minute episodes of jet formation in the Galactic microquasar GRS 1915+105 may sometimes entirely be a superposition of smaller, faster phenomena. We base this conclusion on simultaneous X-ray and infrared…

Astrophysics · Physics 2009-11-10 David M. Rothstein , Stephen S. Eikenberry , Keith Matthews

GS 0836-429 is a neutron star X-ray transient that displays Type-I X-ray bursts. In 2003 and 2004 it experienced two outbursts in X-rays. We present here an analysis of the system bursting properties during these outbursts. We studied the…

High Energy Astrophysical Phenomena · Physics 2016-02-10 E. Aranzana , C. Sánchez-Fernández , E. Kuulkers

We study the dynamical behaviour of the galactic black hole source GX 339-4 during 2002-2011 outbursts using RXTE, Swift(XRT), XMM-Newton(PN) archival data. We present the spectral evolution of the source using four outbursts data and…

High Energy Astrophysical Phenomena · Physics 2019-05-14 U. Aneesha , S. Mandal , H. Sreehari

We study the statistics of soft gamma repeater (SGR) bursts, using a data base of 187 events detected with BATSE and 837 events detected with RXTE PCA, all from SGR 1900+14 during its 1998-1999 active phase. We find that the fluence or…

We report simultaneous observations in the X-ray, infrared, and radio wavelengths of the galactic superluminal source GRS 1915+105. During episodes of rapid disappearance and follow up replenishment of the inner accretion disk evidenced by…

Astrophysics · Physics 2007-05-23 I. F. Mirabel , V. Dhawan , S. Chaty , L. F. Rodriguez , J. Marti , C. R. Robinson , J. Swank , T. Geballe

We report the quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR observations showing spectral state transitions in the neutron star low mass X-ray binary 1RXS J180408.9-342058 during its 2015 outburst. We present results of the analysis of…

High Energy Astrophysical Phenomena · Physics 2020-01-08 M. Fiocchi , A. Bazzano , G. Bruni , R. Ludlam , L. Natalucci , F. Onori , P. Ubertini

The extraordinarily long outburst of GRS 1915+105 makes it one of the most remarkable low-mass X-ray binaries (LMXBs). It has been in a state of constant outburst since its discovery in 1992, an eruption which has persisted ~100 times…

Solar and Stellar Astrophysics · Physics 2010-06-25 P. Deegan , C. Combet , G. A. Wynn

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…

The flux and spectrum of the black hole candidate GX339-4 has been monitored by the Burst and Transient Source Experiment (BATSE) on the Compton Gamma-ray Observatory (CGRO) since the observatory became operational in May 1991. Between the…

Astrophysics · Physics 2009-10-30 B. C. Rubin , B. A. Haron , W. S. Paciesas , C. R. Robinson , S. N. Zhang , G. J. Fishman

We observe strong correlations between the temporal properties of gamma ray bursts (GRBs) and their apparent peak brightness. The strongest effect (with a significance level of 10^{-6}) is the difference between the brightness distributions…

Astrophysics · Physics 2011-07-13 Boris Stern , Juri Poutanen , Roland Svensson

We present a unifying scenario to address the physical origin of the diversity of X-ray lightcurves within the rho variability class of the microquasar GRS 1915+105. This 'heartbeat' state is characterized by a bright flare that recurs…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Joseph Neilsen , Ronald A. Remillard , Julia C. Lee

The Galactic microquasar GRS 1915+105 shows rich variability which is categorized into different classes. In this paper, we report temporal and spectral analysis of GRS 1915+105 to study the properties of the accretion flow when the light…

High Energy Astrophysical Phenomena · Physics 2021-08-04 Anuvab Banerjee , Ayan Bhattacharjee , Debjit Chatterjee , Dipak Debnath , Sandip Kumar Chakrabarti , Tilak Katoch , H. M. Antia

Monitoring with the Ryle Telescope at 15 GHz of the Galactic X-ray transient source GRS 1915+105 has revealed a remarkable range of rapid and extended flares which appear to be related to the X-ray emission as recorded by the RXTE all-sky…

Astrophysics · Physics 2007-05-23 G. G. Pooley , R. P. Fender

(abridged version) We report on ten type I X-ray bursts from GX 17+2 in data obtained with the RXTE/PCA in 1996--2000. Three bursts were short in duration (~10 s), whereas the others lasted for ~6-25 min. Five of the long bursts showed…

Astrophysics · Physics 2009-11-06 E. Kuulkers , J. Homan , M. van der Klis , W. H. G. Lewin , M. Mendez

Aims. The high-redshift (z = 4:048) gamma-ray burst GRB 060206 showed unusual behavior, with a significant rebrightening by a factor of ~ 4 at about 3000 s after the burst. We argue that this rebrightening implies that the central engine…

Astrophysics · Physics 2015-05-13 X. W. Liu , X. F. Wu , T. Lu