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Related papers: Modelling the compact jet in MAXI J1836-194 with d…

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Galactic black hole binaries produce powerful outflows with emit over almost the entire electromagnetic spectrum. Here, we report the first detection with the Herschel observatory of a variable far-infrared source associated with the…

The Galactic transient X-ray binary MAXI~J1836-194 was discovered on 29th August 2011. Here we make a detailed study of the spectral and timing properties of its 2011 outburst using archival data of RXTE Proportional Counter Array…

High Energy Astrophysical Phenomena · Physics 2016-04-15 Arghajit Jana , Dipak Debnath , Sandip K. Chakrabarti , Santanu Mondal , Aslam Ali Molla

The Galactic black hole X-ray binary MAXI J1820+070 had a bright outburst in 2018 when it became the second brightest X-ray source in the Sky. It was too bright for X-ray CCD instruments such as XMM-Newton and Chandra, but was well observed…

LS I +61303 is a gamma-ray binary with periodic radio outbursts coincident with the orbital period of P=26.5 d. The origin of the radio emission is unclear,it could be due either to a jet, as in microquasars, or to the shock boundary…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Massi , Kaufman-Bernado

After 34 years, the black-hole candidate EXO 1846-031 went into outburst again in 2019. We investigate its spectral properties in the hard intermediate and the soft states with NuSTAR and Insight-HXMT. A reflection component has been…

We report on X-ray spectral and timing results of the new black hole candidate (BHC) MAXI J1659-152 with the orbital period of 2.41 hours (shortest among BHCs) in the 2010 outburst from 65 Rossi X-ray Timing Explorer (RXTE) observations and…

We present a broadband spectral and timing study of the black hole candidate MAXI J1803-298 during its 2021 outburst using simultaneous observations from NICER, NuSTAR, and Insight-HXMT. The combined multi-instrument coverage allows us to…

High Energy Astrophysical Phenomena · Physics 2026-05-14 Kaushik Chatterjee , Sujoy K. Nath

We report on a Suzaku observation of the newly discovered X-ray binary MAXI J1836-194. The source is found to be in the hard/intermediate spectral state and displays a clear and strong relativistically broadened iron emission line. We fit…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Rubens C. Reis , Jon M. Miller , Mark T. Reynolds , Andrew C. Fabian , Dominic J. Walton

We explore the coupling between the accretion flow and the jet in black hole X-ray binary (BHXRB) MAXI J1348-630 by analyzing the X-ray and radio observations during its 2019 outburst. We measure the time delay between the radio and…

High Energy Astrophysical Phenomena · Physics 2024-06-25 Bei You , Shuai-kang Yang , Zhen Yan , Xinwu Cao , Andrzej A. Zdziarski

Radio monitoring unveiled late (hundreds to a thousand days) radio flares in a significant fraction of tidal disruption events. We propose that these late-time radio flares are a natural outcome if the surrounding density profile flattens…

High Energy Astrophysical Phenomena · Physics 2024-06-18 Tatsuya Matsumoto , Tsvi Piran

Outflows are common in many astrophysical systems. In the Two Component Advective Flow ({\fontfamily{qcr}\selectfont TCAF}) paradigm which is essentially a generalized Bondi flow including rotation, viscosity and cooling effects, the…

High Energy Astrophysical Phenomena · Physics 2021-10-20 Santanu Mondal , Sandip K. Chakrabarti

We present an in-depth spectral and timing analysis of the Black Hole binary 4U 1630-472 during 2016 and 2018 outbursts as observed by \textit{AstroSat} and \textit{MAXI}. The extensive coverage of the outbursts with \textit{MAXI} is used…

High Energy Astrophysical Phenomena · Physics 2020-07-09 Blessy E. Baby , V. K. Agrawal , Ramadevi M. C. , Tilak Katoch , H. M. Antia , Samir Mandal , Anuj Nandi

The Galactic transient black hole candidate (BHC) MAXI~J1834-021 was detected for the first time by MAXI/GSC on February 05, 2023 and it was active for next $\sim 10$~months. A monotonic evolution of low-frequency QPOs from higher to lower…

High Energy Astrophysical Phenomena · Physics 2025-06-13 Dipak Debnath , Hsiang-Kuang Chang

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…

Many X-ray binaries remain undetected in the mid-infrared, a regime where emission from their compact jets is likely to dominate. Here, we report the detection of the black hole binary GX 339-4 with the Wide-field Infrared Survey Explorer…

Galactic black hole candidate (BHC) XTE~J1118+480 during its 2000 outburst has been studied in a broad energy range using the archival data of PCA and HEXTE payloads of {\it Rossi X-ray Timing Explorer}. Detailed spectral and temporal…

High Energy Astrophysical Phenomena · Physics 2019-05-09 Debjit Chatterjee , Dipak Debnath , Arghajit Jana , Sandip K. Chakrabarti

Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ltimately, how the energy is extracted from the central black hole in radio-loud active…

We report the energy-resolved broadband timing analysis of the black hole X-ray transient MAXI J1631-479 during its 2019 outburst from February 11 to April 9, using data from the Insight-Hard X-ray Modulation Telescope (Insight-HXMT), which…

High Energy Astrophysical Phenomena · Physics 2021-10-04 Q. C. Bu , S. N. Zhang , A. Santangelo , T. M. Belloni , L. Zhang , J. L. Qu , L. Tao , Y. Huang , X. Ma , Z. S. Li , S. Zhang , L. Chen , the Insight-HMXT collaboration

Accretion of black holes at near-Eddington or super-Eddington rates is the most powerful episode that drives black hole growth, and it may work in several types of objects. However, the physics of accretion and jet-disc coupling in such a…

High Energy Astrophysical Phenomena · Physics 2023-05-23 Xiaolong Yang , Su Yao , Luigi C. Gallo , Jun Yang , Luis C. Ho , Minfeng Gu , Willem A. Baan , Jiri Svoboda , Ran Wang , Xiang Liu , Xiaoyu Hong , Xue-Bing Wu , Wei Zhao

We performed shot analyses of X-ray and optical sub-second flares observed during the low/hard state of the 2018 outburst in MAXI J1820$+$070. Optical shots were less spread than X-ray shots. The amplitude of X-ray shots was the highest at…

High Energy Astrophysical Phenomena · Physics 2024-11-07 Mariko Kimura , Hitoshi Negoro , Shinya Yamada , Wataru Iwakiri , Shigeyuki Sako , Ryou Ohsawa