Professor Rob Fender: Publications

An artist's impression of a relativistic jet propagating away from a black hole at close to the speed of light. Such jets are formed by the inner regions of the accretion flow: matter flowing inwards towards the black hole, via processes which are not yet fully understood. The accretion flow emits primarily in X-rays, the relativistic jet in the radio band: by combing observations in each band we can try and understand how such jets form and how much energy they carry away from the black hole.

A refined dynamical mass for the black hole in the X-ray transient XTE J1859+226

(2022)

Authors:

IV Yanes Rizo, MAP Torres, J Casares, SE Motta, T Muñoz-Darias, P Rodríguez-Gil, M Armas Padilla, F Jiménez-Ibarra, PG Jonker, J Corral-Santana, R Fender

Radio observations of the Black Hole X-ray Binary EXO 1846-031 re-awakening from a 34-year slumber

(2022)

Authors:

DRA Williams, SE Motta, R Fender, JCA Miller-Jones, J Neilsen, JR Allison, J Bright, I Heywood, PFL Jacob, L Rhodes, E Tremou, P Woudt, J van den Eijnden, F Carotenuto, DA Green, D Titterington, AJ van der Horst, P Saikia

MeerKAT radio observations of the neutron star low-mass X-ray binary Cen X–4 at low accretion rates

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 516:2 (2022) 2641-2652

Authors:

J van den Eijnden, R Fender, JCA Miller-Jones, TD Russell, P Saikia, GR Sivakoff, F Carotenuto

MeerKAT radio observations of the neutron star low-mass X-ray binary Cen X-4 at low accretion rates

(2022)

Authors:

J van den Eijnden, R Fender, JCA Miller-Jones, TD Russell, P Saikia, GR Sivakoff, F Carotenuto

A Late-time Radio Flare Following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh

The Astrophysical Journal American Astronomical Society 933:2 (2022) 176

Authors:

Itai Sfaradi, Assaf Horesh, Rob Fender, David A Green, David RA Williams, Joe Bright, Steve Schulze

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