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Related papers: RXTE observations and state transition in MAXI J18…

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We report results from the X-ray and optical monitoring of the black hole candidate MAXI J1820+070 (=ASSASN-18ey) over the entire period of its outburst from March to October 2018.In this outburst, the source exhibited two sets of `fast…

High Energy Astrophysical Phenomena · Physics 2019-04-17 Megumi Shidatsu , Satoshi Nakahira , Katsuhiro L. Murata , Ryo Adachi , Nobuyuki Kawai , Yoshihiro Ueda , Hitoshi Negoro

Swift J1734.5-3027 is a hard X-ray transient discovered by Swift while undergoing an outburst in September 2013. Archival observations showed that this source underwent a previous episode of enhanced X-ray activity in May-June 2013. In this…

High Energy Astrophysical Phenomena · Physics 2015-07-01 E. Bozzo , P. Romano , M. Falanga , C. Ferrigno , A. Papitto , H. A. Krimm

Multi-wavelength observations of Galactic black hole transients during outburst decay are instrumental for our understanding of the accretion geometry and the formation of outflows around black hole systems. H1743-322, a black hole…

Astrophysics · Physics 2009-11-13 E. Kalemci , J. A. Tomsick , R. E. Rothschild , K. Pottschmidt , S. Corbel , P. Kaaret

1RXS J180408.9--342058 is a low mass X-ray binary hosting a neutron star, which shows X-ray activity at very different mass-accretion regimes, from very faint to almost the Eddington luminosity. In this work, we present a comprehensive…

High Energy Astrophysical Phenomena · Physics 2019-10-16 A. Marino , M. Del Santo , M. Cocchi , A. D'Aì , A. Segreto , C. Ferrigno , T. Di Salvo , J. Malzac , R. Iaria , L. Burderi

We present a comprehensive spectro-temporal analyses of recurrent outbursting black hole sources GX 339$-$4 and H 1743$-$322 using available AstroSat and NuSTAR archival observations during 2016-2024. The nature of the outburst profiles of…

High Energy Astrophysical Phenomena · Physics 2024-07-18 U. Aneesha , Santabrata Das , Tilak B. Katoch , Anuj Nandi

We present Swift broadband observations of the recently discovered black hole candidate, X-ray transient, XTE J1752-223, obtained over the period of outburst from October 2009 to June 2010. From Swift-UVOT data we confirm the presence of an…

High Energy Astrophysical Phenomena · Physics 2015-05-19 P. A. Curran , T. J. Maccarone , P. Casella , P. A. Evans , W. Landsman , H. A. Krimm , C. Brocksopp , M. Still

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

XTE J1701-407 is a newly discovered X-ray transient source. In this work we investigate its flux variability and study the intermediate long and short bursts discovered by Swift on July 17, and 27, 2008, respectively. So far, only one…

High Energy Astrophysical Phenomena · Physics 2009-11-13 M. Falanga , A. Cumming , E. Bozzo , J. Chenevez

Data accumulated with RXTE during the active state of Cir X-1 as well as during an unusually long transition from the active state to the quiescent state are reported. The long decline from the active state allowed the source…

Astrophysics · Physics 2009-10-30 Hale Bradt , Robert Shirey , Alan Levine

The black hole candidate and X-ray binary MAXI J1535-571 was discovered in September 2017. During the decay of its discovery outburst, and before returning to quiescence, the source underwent at least four reflaring events, with peak…

We have performed a spectral-timing analysis on the black hole X-ray binary MAXI J1535--571 during its 2017 outburst, with the aim of exploring the evolution of the inner accretion flow geometry. X-ray reverberation lags are observed in the…

The neutron star binary SAX J1747.0-2853, located in the Galactic Center region at about 0.5 deg from Sgr A* and at a distance of 9 kpc, has been observed in outburst four times (1998, 1999, 2000 and 2001) by BeppoSAX and RossiXTE. At the…

Astrophysics · Physics 2009-11-10 L. Natalucci , A. Bazzano , M. Cocchi , P. Ubertini , R. Cornelisse , J. Heise , J. J. M. in 't Zand

We present Neutron Star Interior Composition Explorer X-ray and Arcminute Microkelvin Imager Large Array radio observations of a rapid hard-to-soft state transition in the black hole X-ray transient MAXI J1820+070. During the transition…

Here we summarise the Swift broadband observations of the recently discovered X-ray transient and black hole candidate, XTE J1752-223,obtained over the period of outburst from October 2009 to June 2010. We offer a phenomenological treatment…

High Energy Astrophysical Phenomena · Physics 2011-04-06 P. A. Curran , P. Casella , T. J. Maccarone , P. A. Evans , W. Landsman , H. A. Krimm , C. Brocksopp , M. Still

Monitor of All sky X-ray Image (MAXI) discovered a new outburst of an X-ray transient source named MAXI J1421-613. Because of the detection of three X-ray bursts from the source, it was identified as a neutron star low-mass X-ray binary.…

The results of X-ray observations of Galactic superluminal jet source GRS 1915+105 during its low luminosity state and state transitions in October, 1996 - April, 1997 with PCA and HEXTE instruments aboard Rossi X-ray Timing Explorer (RXTE)…

Astrophysics · Physics 2007-05-23 S. Trudolyubov , E. Churazov , M. Gilfanov

We report on optical and RXTE observations of a new high-latitude bursting X-ray transient, XTE J2123-058. We identified the optical counterpart, measured the 5.9573 hr orbital period and constrained the binary inclination and the source…

Astrophysics · Physics 2009-10-31 John A. Tomsick , Jules P. Halpern , Jonathan Kemp , Philip Kaaret

MAXI J1803-298 is a transient black hole candidate discovered in May of 2021 during an outburst that lasted several months. Multiple X-ray observations reveal recurring "dipping" intervals in several of its light curves, particularly during…

During the outbursts of black hole X-ray binaries (BHXRBs), their accretion flows transition through several states. The source luminosity rises in the hard state, dominated by non-thermal emission, before transitioning to the…

We present the results of observations of XTE J0421+560 X-ray transient with Rossi X-ray Timing Explorer in the beginning of April 1998. Lightcurve, obtained by ASM all-sky monitor, shows unusually fast decrease in the object's luminosity.…

Astrophysics · Physics 2007-05-23 M. Revnivtsev , A. Emelyanov , K. Borozdin