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Related papers: Outbursts from IGR J17473-2721

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We present simultaneous, multi-wavelength observations of the Small Magellanic Cloud Be/XRB IGR J01217-7257 (=SXP 2.16) during outbursts in 2014, 2015 and 2016. We also present the results of RXTE observations of the Small Magellanic Cloud…

High Energy Astrophysical Phenomena · Physics 2017-01-18 C. M. Boon , A. J. Bird , M. J. Coe , R. H. D. Corbet , P. A. Evans , J. A. Kennea , H. A. Krimm , S. G. T. Laycock , A. Udalski

We present an analysis of a 37-ks observation of the supergiant fast X-ray transient (SFXT) IGR J17391-3021 (=XTE J1739-302) gathered with Suzaku. The source evolved from quiescence to a low-activity level culminating in three weak flares…

High Energy Astrophysical Phenomena · Physics 2015-05-20 A. Bodaghee , J. A. Tomsick , J. Rodriguez , S. Chaty , K. Pottschmidt , R. Walter , P. Romano

We present optical and infrared monitoring of the 2005 outburst of the halo black hole X-ray transient XTE J1118+480. We measured a total outburst amplitude of ~5.7+-0.1 mag in the R band and ~5 mag in the infrared J, H and K_s bands. The…

In $2016-17$, the Galactic transient black hole candidate GRS 1716-249 exhibited an outburst event after a long period of quiescence of almost 23 years. The source remained in the outbursting phase for $\sim 9$ months. We study the spectral…

High Energy Astrophysical Phenomena · Physics 2021-08-25 Kaushik Chatterjee , Dipak Debnath , Debjit Chatterjee , Arghajit Jana , Sujoy Kumar Nath , Riya Bhowmick , Sandip K. Chakrabarti

In this paper we study the relation of radio emission to X-ray spectral and variability properties for a large sample of black hole X-ray binary systems. This is done to test, refine and extend -- notably into the timing properties -- the…

High Energy Astrophysical Phenomena · Physics 2015-05-13 R. P. Fender , J. Homan , T. M. Belloni

We present the analysis of the high energy emission of the Galactic black hole GRO J1655-40 at the beginning of its 2005 outburst. The data from 458 ks of INTEGRAL observations, spread over 4 weeks, are analyzed, along with the existing…

Astrophysics · Physics 2009-11-13 A. Joinet , E. Kalemci , F. Senziani

We report the discovery of a new hysteresis effect in black hole X-ray binary state transitions, that of the near-infrared (NIR) flux (which most likely originates in the jets) versus X-ray flux. We find, looking at existing data sets, that…

Astrophysics · Physics 2009-06-23 D. M. Russell , T. J. Maccarone , E. G. Koerding , J. Homan

A large radio outburst from Sgr A* was observed during the VLA weekly monitoring program at 2 cm, 1.3 cm and 7 mm, nearly coincident with the brightest X-ray flare detected to date with the XMM-Newton X-ray Observatory on 2002-10-03. The…

Astrophysics · Physics 2009-11-10 Jun-Hui Zhao , R. M. Herrnstein , G. C. Bower , W. M. Goss , S. M. Liu

MAXI J1807+132 is an X-ray transient discovered during the decay of an outburst in 2017. We present optical and X-ray monitoring of the source over more than 125 days, from outburst to quiescence. The outburst decay is characterized by the…

High Energy Astrophysical Phenomena · Physics 2018-12-26 F. Jiménez-Ibarra , T. Muñoz-Darias , M. Armas Padilla , D. M. Russell , J. Casares , M. A. P. Torres , D. Mata Sánchez , P. G. Jonker , F. Lewis

The magnetar SGR J1935+2154 entered a new active episode on October 10, 2022, with X-ray bursts and enhanced persistent emission. At the tail of high burst rate interval, lasting several hours, radio bursts were detected, revealing the…

High Energy Astrophysical Phenomena · Physics 2025-01-14 Fu Yu-Cong , Lin Lin , Ge Ming-Yu , Enoto Teruaki , Hu Chin-Ping , Younes George , Göğüş Ersin , Malacaria Christian

We investigate the early phase of the first state change during the 2008 September-November outburst of H1743-322, first detected by the INTEGRAL satellite. We analyse INTEGRAL, RXTE, Swift, and XMM/Newton observations, which provide…

High Energy Astrophysical Phenomena · Physics 2009-11-13 L. Prat , J. Rodriguez , M. Cadolle Bel , E. Kuulkers , M. Hanke , J. Tomsick , S. Corbel , M. Coriat , J. Wilms , A. Goldwurm

IGR J17407-2808 is an enigmatic and poorly studied X-ray binary that was recently observed quasi-simultaneously with NuSTAR and XMM-Newton. In this paper we report the results of this observational campaign. During the first 60 ks of…

High Energy Astrophysical Phenomena · Physics 2023-06-14 L. Ducci , C. Malacaria , P. Romano , E. Bozzo , M. Berton , A. Santangelo , E. Congiu

We have performed a statistical study of the properties of 110 bright X-ray outbursts in 36 low-mass X-ray binary transients (LMXBTs) seen with the All-Sky Monitor (2--12 keV) on board the {\it Rossi X-ray Timing Explorer} ({\it RXTE}) in…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Zhen Yan , Wenfei Yu

We report striking changes in the broadband spectrum of the compact jet of the black hole transient MAXI J1836-194 over state transitions during its discovery outburst in 2011. A fading of the optical-infrared (IR) flux occurred as the…

We present the results of detailed analysis of X-ray data in 3-20 keV range from a ~70 day outburst of the neutron star transient Aquila X-1 during September-November 2000. Optical monitoring with the YALO 1m telescope was used to trigger…

Astrophysics · Physics 2009-11-10 D. Maitra , C. D. Bailyn

We report on two short XMM-Newton observations performed in August 2006 and February 2007 during the quiescence state of the enigmatic black hole candidate system IGR J17091-3624. During both observations the source was clearly detected.…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Rudy Wijnands , Yi Jung Yang , Diego Altamirano

We have studied the hard X-ray variability of the soft X-ray transient GRO J0422+32 with BATSE in the 20-100 keV energy band. Our analysis covers 180 days following the first X-ray detection of the source on 1992 August 5, fully covering…

We have obtained simultaneous optical and near infrared observations of 4U 1543-47 during its 2002 outburst. The most striking feature of the outburst light curve is the secondary maximum which appears after the object transitions into the…

Astrophysics · Physics 2009-11-10 M. M. Buxton , C. D. Bailyn

Aims: Hete J1900.1-2455 is the seventh known X-ray transient accreting millisecond pulsar and has been in outburst for more than one year. We compared the data on Hete J1900.1-2455 with other similar objects and made an attempt at deriving…

We report on INTEGRAL observations performed during the 2004 outburst of the bright black hole transient GX 339-4. We analysed IBIS and JEM-X public data starting on 9th August and lasting about one month. During this period GX 339-4 showed…

Astrophysics · Physics 2008-11-26 M. Del Santo , J. Malzac , P. Ubertini , T. Belloni
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