collaborators

6 papers

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…

astro-ph.HE2026

Cosmic rays, gamma rays and neutrinos from discrete black hole X-ray binary ejecta

Nicolas J. Bacon, Alex J. Cooper, Dimitrios Kantzas +2

The origin of cosmic rays from outside the Solar system are unknown, as they are deflected by the interstellar magnetic field. Supernova remnants are the main candidate for cosmic…

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.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

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.HE2025

Joint Radiative and Kinematic Modelling of X-ray Binary Ejecta: Energy Estimate and Reverse Shock Detection

A. J. Cooper, J. H. Matthews, F. Carotenuto +6

Black hole X-ray binaries in outburst launch discrete, large-scale jet ejections which can propagate to parsec scales. The kinematics of these ejecta appear to be well described by…