activity
20162026
most citedDiscovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds

169 citations · 529 across the 36 of their papers we have counts for

collaborators
Showing 2026Show all

8 papers · 1 filter

astro-ph.HE2026

mm-jets in the multi-messenger era

Karri I. I. Koljonen, Thomas D. Russell, Britton Jeter +16

Jets and outflows operate across the full cosmic mass scale from young stellar objects (YSOs) and X-ray binaries (XRBs) to active galactic nuclei (AGN), gamma-ray bursts (GRBs), an…

astro-ph.IM2026

Understanding cosmic explosions

Karri I. I. Koljonen, Tomek Kamiński, Anna Y. Q. Ho +11

Millimeter-wavelength observations provide a uniquely sensitive window into the physics of cosmic explosions, from supernovae (SNe) and tidal disruption events (TDEs) to nova erupt…

astro-ph.HE2026

A Multi-Wavelength Picture of the Surprisingly Short 2024/25 Outburst from EXO 0748-676

Amy H. Knight, Lauren Rhodes, Noel Castro Segura +11

After sixteen years in quiescence, EXO 0748-676 unexpectedly returned to outburst in March 2024. However, in stark contrast to its previous outburst (1985 - 2008), EXO 0748-676 ret…

astro-ph.HE2026

A Galactic microblazar as a potential accelerator of ultra-high-energy particles

Josep Martí, Pedro L. Luque-Escamilla, Benito Marcote +10

Context. Persistent jets from X-ray binaries which are aligned very close to the line of sight could be considered to be Galactic equivalents of blazars, or 'microblazars'. They ar…

astro-ph.SR2026

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry

J. van den Eijnden, L. Kaper

Bow shocks are one the most commonly observed impact sites of massive star feedback. Their existence is often taken as evidence of the supersonic motion or even runaway nature of t…

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

Detection of an Extremely Luminous Radio Counterpart to the Be/X-ray Binary A0538-66

Justine Crook-Mansour, Rob Fender, Alex Andersson +14

We present the discovery of radio emission from the Be/X-ray binary A0538-66 with the Australian Square Kilometre Array Pathfinder (ASKAP), and results from a subsequent weekly mon…

astro-ph.HE2026

Dynamic shocks powered by a wide, relativistic, super-Eddington outflow launched by an accreting neutron star in the mid-20th century

F. J. Cowie, R. P. Fender, I. Heywood +11

Accreting systems can launch powerful outflows which interact with the surrounding medium. We combine new radio observations of the accreting neutron star X-ray binary (XRB) Circin…