activity
20062022
most citedCygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds

285 citations · 1.4k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.HE2022★ 16 cited

Comprehensive coverage of particle acceleration and kinetic feedback from the stellar mass black hole V404 Cygni

R. P. Fender, K. P. Mooley, S. E. Motta +8

We present analysis of comprehensive radio observations of the black hole V404 Cyg during its 2015 outburst. These data represent the best ever coverage of jet production and parti…

astro-ph.HE2021★ 285 cited

Cygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds

James C. A. Miller-Jones, Arash Bahramian, Jerome A. Orosz +23

The evolution of massive stars is influenced by the mass lost to stellar winds over their lifetimes. These winds limit the masses of the stellar remnants (such as black holes) that…

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.HE2017★ 87 cited

Extreme Jet Ejections from the Black Hole X-ray Binary V404 Cygni

A. J. Tetarenko, G. R. Sivakoff, J. C. A Miller-Jones +14

We present simultaneous radio through sub-mm observations of the black hole X-ray binary (BHXB) V404 Cygni during the most active phase of its June 2015 outburst. Our hour long…

astro-ph.HE2017★ 45 cited

Resolved, expanding jets in the Galactic black hole candidate XTE J1908+094

A. P. Rushton, J. C. A. Miller-Jones, P. A. Curran +15

Black hole X-ray binaries undergo occasional outbursts caused by changing inner accretion flows. Here we report high-angular resolution radio observations of the 2013 outburst of t…

astro-ph.HE2016★ 47 cited

The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations

G. E. Anderson, A. Horesh, K. P. Mooley +12

We present a radio light curve of supernova (SN) 2014C taken with the Arcminute Microkelvin Imager (AMI) Large Array at 15.7 GHz. Optical observations presented by Milisavljevic et…