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We present the results of our observations of the early stages of the 2012--2013 outburst of the transient black hole X-ray binary (BHXRB), Swift J1745$-$26, with the VLA, SMA, and JCMT (SCUBA--2). Our data mark the first multiple-band mm &…

Jets from accreting black hole (BH) X-ray binaries (XRBs) are powerful outflows that release a large fraction of the accretion energy to the surrounding environment, providing a feedback mechanism that may alter the interstellar medium…

High Energy Astrophysical Phenomena · Physics 2025-09-15 I. Mariani , S. E. Motta , P. Atri , J. H. Matthews , R. P. Fender , J. Martí , P. L. Luque-Escamilla , I. Heywood

MAXI J1535-571 is a Galactic black hole candidate X-ray binary that was discovered going into outburst in 2017 September. In this paper, we present comprehensive radio monitoring of this system using the Australia Telescope Compact Array…

The fast variability observed in the X-ray emission from black-hole binaries has a very complex phenomenology, but offers the possibility to investigate directly the properties of the inner accretion flow. In particular, type-B oscillations…

High Energy Astrophysical Phenomena · Physics 2020-07-08 Tomaso M. Belloni , Liang Zhang , Nikolaos D. Kylafis , Pablo Reig , Diego Altamirano

The search and study of close pairs of supermassive black holes (SMBHs) is important in the study of galaxy mergers which can possibly trigger active galactic nucleus (AGN) activity, and in the context of their evolution into the…

Astrophysics of Galaxies · Physics 2019-03-06 Sumit Jaiswal , Prashanth Mohan , Tao An , Sándor Frey

We have discovered an X-ray jet due to material ejected from the black hole X-ray transient XTE J1550-564. The discovery was first reported by Corbel et al. (Science, 298, 196 and astro-ph/0210224), and here, we present an analysis of the…

The recently discovered Galactic X-ray transient XTE J1752-223 entered its first known outburst in 2010, emitting from the X-ray to the radio regimes. Its general X-ray properties were consistent with those of a black hole candidate in…

High Energy Astrophysical Phenomena · Physics 2015-05-19 J. Yang , C. Brocksopp , S. Corbel , Z. Paragi , T. Tzioumis , R. P. Fender

We report on ALMA continuum observations of the black hole X-ray binary A0620-00, at an X-ray luminosity nine orders of magnitude sub-Eddington. The system was significantly detected at 98 GHz (at $44 \pm 7~\mu{\rm Jy}$) and only marginally…

We describe the first complete polarimetric dataset of the entire outburst of a low-mass black hole X-ray binary system and discuss the constraints for geometry and radiative mechanisms it imposes. During the decaying hard state, when the…

The black hole candidate, XTE J1752-223, was discovered in 2009 October when it entered an outburst. We obtained radio data from the Australia Telescope Compact Array for the duration of the ~9 month event. The lightcurves show that the…

High Energy Astrophysical Phenomena · Physics 2015-12-02 Catherine Brocksopp , Stephane Corbel , Tasso Tzioumis , Jess Broderick , Jerome Rodriguez , Jun Yang , Rob Fender , Zsolt Paragi

Black holes in binary systems execute patterns of outburst activity where two characteristic X-ray states are associated with different behaviours observed at radio wavelengths. The hard state is associated with radio emission indicative of…

We report the results of fitting Insight-HXMT data to the black hole X-ray binary MAXI J1348-430, which was discovered on January 26th, 2019, with the Gas Slit Camera (GSC) on-board MAXI. Several observations at the beginning of the first…

High Energy Astrophysical Phenomena · Physics 2023-10-30 Yujia Song , Nan Jia , Jun Yang , Ye Feng , Lijun Gou , Tianhua Lu

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

MAXI J1305-704 has been proposed as a high-inclination candidate black hole X-ray binary in view of its X-ray properties and dipping behaviour during outburst. We present photometric and spectroscopic observations of the source in…

High Energy Astrophysical Phenomena · Physics 2021-06-30 D. Mata Sánchez , A. Rau , A. Álvarez Hernández , T. F. J. van Grunsven , M. A. P. Torres , P. G. Jonker

In this paper we study the wind accretion onto a rotating black hole in the close binary system harboring a young massive star. It is shown that the angular momentum of the accreted stellar wind material is not sufficient for the formation…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Maxim V. Barkov , Dmitry V. Khangulyan

Supermassive black holes (SMBHs) can capture and tidally disrupt stars or sub-stellar objects orbiting nearby. The detections of Sw J1644+57-like events suggest that at least some TDEs can launch a relativistic jet beaming towards Earth. A…

High Energy Astrophysical Phenomena · Physics 2015-12-25 Wei-Hua Lei , Qiang Yuan , Bing Zhang , Q. Daniel Wang

The black hole candidate MAXI J1348-630 was discovered on January 26th, 2019, with the Gas Slit Camera (GSC) on-board \textit{MAXI}. We report a detailed spectral analysis of this source by using the archived data of \textit{NuSTAR}. A…

High Energy Astrophysical Phenomena · Physics 2022-02-16 Nan Jia , Xueshan Zhao , Lijun Gou , Javier A. Garcia , Zhenxuan Liao , Ye Feng , Yufeng Li , Yuan Wang , Huixian Li , Jianfeng Wu

We present observations by the Fermi Gamma-Ray Space Telescope Gamma-Ray Burst Monitor (GBM) of the nearby (z=0.55) GRB 101219B. This burst is a long GRB, with an associated supernova and with a blackbody component detected in the early…

High Energy Astrophysical Phenomena · Physics 2015-06-23 J. Larsson , J. L. Racusin , J. M. Burgess

We present Very Long Baseline Interferometry (VLBI) observations of the high mass X-ray binary LSI+61303, carried out with the European VLBI Network (EVN). Over the 11 hour observing run, performed 10 days after a radio outburst, the radio…

Astrophysics · Physics 2007-05-23 M. Massi , M. Ribo , J. M. Paredes , M. Peracaula , R. Estalella

{\it Chandra} spectroscopy of transient stellar-mass black holes in outburst has clearly revealed accretion disk winds in soft, disk--dominated states, in apparent anti-correlation with relativistic jets in low/hard states. These disk winds…