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Related papers: Accretion geometry of the black hole binary MAXI J…

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The inner radius of the accretion disc around a black hole in the low/hard state can be measured in one of two ways. Firstly, via the extent of broadening of the iron emission line, and secondly, from the luminosity and temperature of the…

High Energy Astrophysical Phenomena · Physics 2015-06-17 M. Kolehmainen , C. Done , M. Diaz Trigo

We present an analysis of the whole 2018 outburst of the black hole X-ray binary MAXI J1820+070 with Insight-HXMT data. We focus our study on the temporal evolution of the parameters of the source. We employ two different models to fit the…

High Energy Astrophysical Phenomena · Physics 2024-07-03 Ningyue Fan , Songyu Li , Rui Zhan , Honghui Liu , Zuobin Zhang , Cosimo Bambi , Long Ji , Xiang Ma , James F. Steiner , Shuang-Nan Zhang , Menglei Zhou

We have compared the 2001 XMM-Newton spectra of the stellar mass black hole binary XTE J1650-500 and the active galaxy MGC-6-30-15, focusing on the broad, excess emission features at ~4--7 keV displayed by both sources. Such features are…

High Energy Astrophysical Phenomena · Physics 2015-06-04 D. J. Walton , R. C. Reis , E. M. Cackett , A. C. Fabian , J. M. Miller

X-rays are emitted from the corona above the orbiting matter of the accretion disk and travel either directly to us or illuminate the disk. This illumination of the inner disk is enhanced by gravitational light bending, which focuses the…

High Energy Astrophysical Phenomena · Physics 2026-04-27 William Surgent , Daniel R. Wilkins

In most accreting black-hole systems the copious X-rays commonly observed from the inner-most regions are accompanied by a reflection spectrum. The latter is the signature of energetic photons reprocessed by the optically thick material of…

High Energy Astrophysical Phenomena · Physics 2018-05-03 J. A. García , T. R. Kallman , M. Bautista , C. Mendoza , J. Deprince , P. Palmeri , P. Quinet

We present multi-wavelength fast timing observations of the black hole X-ray binary MAXI J1820+070 (ASASSN-18ey), taken with the Karl G. Jansky Very Large Array (VLA), Atacama Large Millimeter/Sub-Millimeter Array (ALMA), Very Large…

We analyse the X-ray spectrum of the black hole X-ray binary MAXI J1820+070 using observations from XMM-Newton and NuSTAR during 'hard' states of its 2018-2019 outburst. We take a fully Bayesian approach, and this is one of the first papers…

High Energy Astrophysical Phenomena · Physics 2024-02-20 Sachin D. Dias , Simon Vaughan , Mehdy Lefkir , Graham Wynn

We present a detailed timing analysis of the bright black hole X-ray binary MAXI J1820+070 (ASASSN-18ey), during its first detected outburst lasting from March 2018 until October 2019 based on Swift/XRT window timing mode observations,…

High Energy Astrophysical Phenomena · Physics 2020-02-12 H. Stiele , A. K. H. Kong

We analyzed simultaneous archival XMM-Newton and RXTE observations of the X-ray binary and black hole candidate Swift J1753.5-0127. In a previous analysis of the same data a soft thermal component was found in the X-ray spectrum, and the…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Beike Hiemstra , Paolo Soleri , Mariano Mendez , Tomaso Belloni , Reham Mostafa , Rudy Wijnands

Understanding the dynamics behind black hole state transitions and the changes they reflect in outbursts has become long-standing problem. The X-ray reflection spectrum describes the interaction between the hard X-ray source (the power-law…

High Energy Astrophysical Phenomena · Physics 2015-06-19 D. S. Plant , R. P. Fender , G. Ponti , T. Muñoz-Darias , M. Coriat

We present the results of our quasi-simultaneous radio, sub-mm, infrared, optical and X-ray study of the Galactic black hole candidate X-ray binary MAXI J1836-194 during its 2011 outburst. We consider the full multi-wavelength spectral…

High Energy Astrophysical Phenomena · Physics 2015-06-18 T. D. Russell , R. Soria , J. C. A. Miller-Jones , P. A. Curran , S. Markoff , D. M. Russell , G. R. Sivakoff

(Abridged) Recent XMM-Newton studies of X-ray variability in the hard states of black hole X-ray binaries (BHXRBs) imply that the variability is generated in the 'standard' optically-thick accretion disc. The variability originates in the…

High Energy Astrophysical Phenomena · Physics 2015-06-11 P. Cassatella , P. Uttley , T. J. Maccarone

We report on simultaneous sub-second optical and X-ray timing observations of the low mass X-ray binary black hole candidate MAXI J1820+070. The bright 2018 outburst rise allowed simultaneous photometry in five optical bands ($ugriz_s$)…

We present the results of spectral fits made to 57 pointed observations of the Galactic black hole candidate and X-ray transient XTE J1650-500, made with the Rossi X-ray Timing Explorer in 2001 when the source was in a transition from the…

Astrophysics · Physics 2009-11-11 Sabrina Rossi , Jeroen Homan , Jon M. Miller , Tomaso Belloni

We report on the Insight-HXMT observations of the new black hole X-ray binary MAXI J1820+070 during its 2018 outburst. Detailed spectral analysis via the continuum fitting method shows an evolution of the inferred spin during its high soft…

We study the evolution of the temporal properties of MAXI 1820+070 during the 2018 outburst in its hard state from MJD 58190 to 58289 with Insight-HXMT in a broad energy band 1-150 keV. We find different behaviors of the hardness ratio, the…

We present 6.4 keV iron K-alpha fluorescent line profiles predicted for a relativistic black hole accretion disk in the presence of a spiral motion in Kerr geometry, the work extended from an earlier literature motivated by recent…

Astrophysics · Physics 2011-05-10 Keigo Fukumura , Sachiko Tsuruta

X-ray spectroscopy of galactic black hole binaries serve as a powerful tool to gain an overall understanding of the system. Not only can the properties of the accretion disk be studied in detail, the fundamental properties of the black hole…

High Energy Astrophysical Phenomena · Physics 2023-02-16 Sandeep K. Rout , Santosh Vadawale , Javier Garcia , Riley Connors

We study the outbursts of the black hole X-ray binaries MAXI J1659-152, SWIFT J1753.5--0127 and GX 339-4 with the Swift X-ray Telescope. The bandpass of the X-ray Telescope has access to emission from both components of the accretion flow:…

High Energy Astrophysical Phenomena · Physics 2015-06-23 M. Kalamkar , M. T. Reynolds , M. van der Klis , D. Altamirano , J. M. Miller

The black-hole X-ray transient MAXI J1820+07 (=ASSASN-18ey) discovered in March 2018 was one of the optically brightest ever seen, which has resulted in very detailed optical outburst light-curves being obtained. We combine them here with…