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20112026
most citedThe faint "heartbeats" of IGR J17091-3624: an exceptional black-hole candidate

159 citations · 241 across the 22 of their papers we have counts for

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astro-ph.HE2026

Accreting Neutron Stars in Low-Mass X-ray Binaries

M. C. Baglio, S. E. Motta, A. P. Nitindala +1

Neutron star low-mass X-ray binaries (NS LMXBs) are systems in which a neutron star accretes matter from a Roche-lobe-filling companion via an accretion disc, releasing gravitation…

astro-ph.HE2026

Spectropolarimetric detection of baryonic mass loading in a transient relativistic jet: application to the black hole X-ray binary Swift J1727.81613

A. K. Hughes, R. P. Fender, G. R. Sivakoff +10

Radio emission during X-ray binary outbursts is dominated by synchrotron radiation from relativistic jets, but is usually studied through total-intensity diagnostics such as flux d…

astro-ph.HE2026

Transforming X-ray Binary Astrophysics with SKA+VLBI

Tao An, Ailing Wang, James C. A. Miller-Jones +6

X-ray binaries (XRBs) are unique laboratories where accretion, jets, strong gravity and magnetic fields can be probed on humanly tractable timescales. The phased SKA-Mid operating…

astro-ph.HE2026

Accreting Compact Object Binaries with the SKA

Aru Beri, Francesco Carotenuto, Rob P. Fender +4

Accreting binary systems provide a time-resolved view of the accretion and ejection processes that are seen in all classes of compact objects, from stellar-mass to supermassive. Th…

astro-ph.HE2026

The link between obscured accretion and mildly relativistic precessing jets

Rob Fender, Sara Motta

We have recently shown evidence that the most relativistic jets (with Lorentz factor >2) from stellar-mass black holes in X-ray binary systems may be locked to a fixed axis, likely…

astro-ph.HE2026

On The Nature of Einstein Probe Transient EP250916a: Insights from X-ray, Optical, and Radio Observations

Gaurava K. Jaisawal, Giulia Illiano, Francesco Carotenuto +7

We report multi-wavelength studies of the transient EP250916a, detected by the Einstein Probe on 2025 September 16. Located at low Galactic latitude, the source exhibited a rapid X…

astro-ph.HE2026

The Homogeneous MeerKAT and Swift/XRT X-ray Binary Radio:X-ray Plane

Justine Crook-Mansour, Rob Fender, Andrew Hughes +22

During the hard and quiescent spectral states in X-ray binaries, a non-linear correlation is observed between radio and X-ray luminosities, providing a valuable tool to probe the c…

astro-ph.HE2026

Multi-wavelength outburst activity from EP J174942.2-384834: a very faint X-ray transient discovered by Einstein Probe

F. Coti Zelati, A. Marino, Y. L. Wang +27

We report the discovery and multi-wavelength characterization of the Galactic transient EP J174942.2384834, first detected by the Einstein Probe during a faint X-ray outburst in…

astro-ph.HE2026

Exploring the potential for ultra-relativistic jets in Scorpius X-1 with low angular resolution radio observations

I. Stephens, L. Rhodes, A. J. Cooper +2

Scorpius X-1 (Sco X-1) is a neutron star X-ray binary in which the neutron star is accreting rapidly from a low mass stellar companion. At radio frequencies, Sco X-1 is highly lumi…

astro-ph.HE2026★ 4 cited

Large-scale radio bubbles around the black hole transient V4641 Sgr

Noa Grollimund, Stéphane Corbel, Rob Fender +7

Black holes (BHs) in microquasars can launch powerful relativistic jets that have the capacity to travel up to several parsecs from the compact object and interact with the interst…

astro-ph.HE2025★ 1 cited

A MeerKAT view of the parsec-scale jets in the black-hole X-ray binary GRS 1758-258

I. Mariani, S. E. Motta, P. Atri +5

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 fe…

astro-ph.HE2025

An ultraviolet burst oscillation candidate from the low-mass X-ray binary EXO 0748-676

A. Miraval Zanon, F. Ambrosino, G. Illiano +15

X-ray burst oscillations are quasi-coherent periodic signals at frequencies close to the neutron star spin frequency. They are observed during thermonuclear Type I X-ray bursts fro…

astro-ph.HE2025

Relativistic precessing jets powered by an accreting neutron star

F. J. Cowie, R. P. Fender, I. Heywood +9

Precessing relativistic jets launched by compact objects are rarely directly measured, and present an invaluable opportunity to better understand many features of astrophysical jet…

astro-ph.HE2025

A relativistic jet from a neutron star breaking out of its natal supernova remnant

K. V. S. Gasealahwe, K. Savard, I. M. Monageng +10

The young neutron star X-ray binary, Cir X-1, resides within its natal supernova remnant and experiences ongoing outbursts every 16.5 days, likely due to periastron passage in an e…

astro-ph.HE2025★ 3 cited

The Accretion-Ejection Connection in the Black Hole X-ray Binary MAXI J1820070

Joe S. Bright, Rob Fender, David M. Russell +12

The black hole X-ray binary MAXI J1820070 began its first recorded outburst in March 2018, and remained an active radio, X-ray, and optical source for over four years. Due to th…

astro-ph.HE2025★ 14 cited

MeerKAT discovers a jet-driven bow shock near GRS 1915+105. How an invisible large-scale jet sculpts a microquasar's environment

S. E. Motta, P. Atri, James H. Matthews +5

Black holes, both supermassive and stellar-mass, impact the evolution of their surroundings on a large range of scales. While the role of supermassive black holes is well studied,…

astro-ph.HE2025★ 9 cited

Quantifying jet-interstellar medium interactions in Cyg X-1: Insights from dual-frequency bow shock detection with MeerKAT

P. Atri, S. E. Motta, Jakob van den Eijnden +6

Accretion and outflows are astrophysical phenomena observed across a wide range of objects, from white dwarfs to supermassive black holes. Developing a complete picture of these pr…

astro-ph.HE2025★ 3 cited

Jets from a stellar-mass black hole are as relativistic as those from supermassive black holes

Xian Zhang, Wenfei Yu, Francesco Carotenuto +15

Relativistic jets from supermassive black holes in active galactic nuclei are amongst the most powerful phenomena in the universe, acting to regulate the growth of massive galaxies…

astro-ph.HE2025

Blast waves and reverse shocks: from ultra-relativistic GRBs to moderately relativistic X-ray binaries

James H. Matthews, Alex J. Cooper, Lauren Rhodes +8

Blast wave models are commonly used to model relativistic outflows from ultra-relativistic gamma-ray bursts (GRBs), but are also applied to lower Lorentz factor ejections from X-ra…

astro-ph.HE2024★ 4 cited

Polarized multiwavelength emission from pulsar wind - accretion disk interaction in a transitional millisecond pulsar

M. C. Baglio, F. Coti Zelati, A. Di Marco +17

Transitional millisecond pulsars (tMSPs) bridge the evolutionary gap between accreting neutron stars in low-mass X-ray binaries and millisecond radio pulsars. These systems exhibit…

astro-ph.HE2011★ 159 cited

The faint "heartbeats" of IGR J17091-3624: an exceptional black-hole candidate

D. Altamirano, T. Belloni, M. Linares +9

We report on the first 180 days of RXTE observations of the outburst of the black hole candidate IGR J17091-3624. This source exhibits a broad variety of complex light curve patter…