activity
20122026
most citedNine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus

295 citations · 1.9k across the 28 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2026

The Nearest Galactic Nucleus: Studying the Galactic Centre with SKA-Mid

Rainer Schoedel, Antxon Alberdi, Izaskun Jiménez-Serra +24

The Galactic Centre is the nearest nucleus of a galaxy and the most extreme environment that we can observe down to physical scales of a few hundred astronomical units. There is no…

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★ 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

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

Relativistic ejecta from stellar mass black holes: insights from simulations and synthetic radio images

Katie Savard, James H. Matthews, Rob Fender +1

We present numerical simulations of discrete relativistic ejecta from an X-ray binary (XRB) with initial conditions directly informed by observations. XRBs have been observed to la…

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.GA2024★ 2 cited

The SKA Galactic Centre Survey -- A White Paper

Rainer Schoedel, Antxon Alberdi, Izaskun Jimenez-Serra +17

With its extreme density of stars and stellar remnants, dense young massive clusters, high specific star formation rate, intense radiation field, high magnetic field strength, and…

astro-ph.HE2021★ 15 cited

MeerKAT discovery of radio emission from the Vela X-1 bow shock

J. van den Eijnden, I. Heywood, R. Fender +7

Vela X-1 is a runaway X-ray binary system hosting a massive donor star, whose strong stellar wind creates a bow shock as it interacts with the interstellar medium. This bow shock h…

astro-ph.HE2021★ 50 cited

Observations of a radio-bright, X-ray obscured GRS 1915+105

S. E. Motta, J. J. E. Kajava, M. Giustini +9

The Galactic black hole transient GRS1915+105 is famous for its markedly variable X-ray and radio behaviour, and for being the archetypal galactic source of relativistic jets. It e…

astro-ph.HE2020★ 226 cited

Observation of inverse Compton emission from a long -ray burst

V. A. Acciari, S. Ansoldi, L. A. Antonelli +301

Long-duration gamma-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterised by an initial phase o…

astro-ph.HE2020★ 132 cited

An extremely powerful long-lived superluminal ejection from the black hole MAXI J1820+070

J. S. Bright, R. P. Fender, S. E. Motta +25

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. Th…

astro-ph.HE2020★ 25 cited

Radio & X-ray detections of GX 339--4 in quiescence using MeerKAT and Swift

E. Tremou, S. Corbel, R. P. Fender +12

The radio:X-ray correlation that characterises accreting black holes at all mass scales - from stellar mass black holes in binary systems to super-massive black holes powering Acti…

astro-ph.GA2019★ 3 cited

Cosmic-ray Particles in the Galactic Center: Blowing in the Wind

F. Yusef-Zadeh, M. Wardle, I. Heywood +2

Recent results from multi-wavelength observations of the inner few hundred pc of the Galactic center have added two new characteristics to the ISM in this unique region. One is the…

astro-ph.HE2019★ 31 cited

The 2018 outburst of BHXB H1743-322 as seen with MeerKAT

D. R. A. Williams, S. E. Motta, R. Fender +11

In recent years, the black hole candidate X-ray binary system H1743-322 has undergone outbursts and it has been observed with X-ray and radio telescopes. We present 1.3 GHz MeerKAT…

astro-ph.GA2019★ 150 cited

Inflation of 430-parsec bipolar radio bubbles in the Galactic Centre by an energetic event

I. Heywood, F. Camilo, W. D. Cotton +96

The Galactic Centre contains a supermassive black hole with a mass of 4 million suns within an environment that differs markedly from that of the Galactic disk. While the black hol…

astro-ph.HE2019★ 295 cited

Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus

G. Miniutti, R. D. Saxton, M. Giustini +11

In the past two decades, high amplitude electromagnetic outbursts have been detected from dormant galaxies and often attributed to the tidal disruption of a star by the central bla…

astro-ph.HE2019★ 113 cited

Disk-jet coupling in the 2017/2018 outburst of the Galactic black hole candidate X-ray binary MAXI J1535-571

T. D. Russell, A. J. Tetarenko, J. C. A. Miller-Jones +19

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 o…

astro-ph.HE2018★ 156 cited

A Strong Jet Signature in the Late-Time Lightcurve of GW170817

K. P. Mooley, D. A. Frail, D. Dobie +19

We present new 0.6-10 GHz observations of the binary neutron star merger GW170817 covering the period up to 300 days post-merger, taken with the Karl G. Jansky Very Large Array, th…

astro-ph.HE2017★ 28 cited

ThunderKAT: The MeerKAT Large Survey Project for Image-Plane Radio Transients

R. Fender, P. A. Woudt, R. Armstrong +59

ThunderKAT is the image-plane transients programme for MeerKAT. The goal as outlined in 2010, and still today, is to find, identify and understand high-energy astrophysical process…

astro-ph.CO2013★ 5 cited

Ground-state 12CO emission and a resolved jet at 115 GHz (rest-frame) in the radio loud quasar 3C318

Ian Heywood, Alejo Martinez-Sansigre, Chris J. Willott +1

An analysis of 44 GHz VLA observations of the z = 1.574 radio-loud quasar 3C318 has revealed emission from the redshifted J = 1 - 0 transition of the CO molecule and spatially reso…

astro-ph.HE2013★ 52 cited

The closest black holes

Rob Fender, Tom Maccarone, Ian Heywood

Starting from the assumption that there is a large population (> 10^8) of isolated, stellar-mass black holes (IBH) distributed throughout our galaxy, we consider the detectable sig…

astro-ph.IM2012

Future Science Prospects for AMI

Keith Grainge, Paul Alexander, Richard Battye +72

The Arcminute Microkelvin Imager (AMI) is a telescope specifically designed for high sensitivity measurements of low-surface-brightness features at cm-wavelength and has unique, im…