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.

On the distance to the black hole X-ray binary Swift J1727.8$-$1613

(2025)

Authors:

Benjamin J Burridge, James CA Miller-Jones, Arash Bahramian, Steve R Prabu, Reagan Streeter, Noel Castro Segura, Jesús M Corral Santana, Christian Knigge, Evangelia Tremou, Francesco Carotenuto, Rob Fender, Payaswini Saikia

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The Observed Phase Space of Mass-loss History from Massive Stars Based on Radio Observations of a Large Supernova Sample

The Astrophysical Journal American Astronomical Society 979:2 (2025) 189

Authors:

Itai Sfaradi, Assaf Horesh, Rob Fender, Lauren Rhodes, Joe Bright, David Williams-Baldwin, Dave A Green

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Type I X-ray Bursts Reflected During the X-ray Eclipses of EXO 0748-676

(2025)

Authors:

Amy H Knight, Jakob van den Eijnden, Adam Ingram, James H Matthews, Sara E Motta, Matthew Middleton, Giulio C Mancuso, Douglas JK Buisson, Diego Altamirano, Rob Fender, Timothy P Roberts

More details from the publisher

The observed phase space of mass-loss history from massive stars based on radio observations of a large supernova sample

(2025)

Authors:

Itai Sfaradi, Assaf Horesh, Rob Fender, Lauren Rhodes, Joe Bright, David Williams-Baldwin, Dave A Green

More details from the publisher

State-dependent signatures of jets and winds in the optical and infrared spectrum of the black hole transient GX 339$-$4

(2025)

Authors:

A Ambrifi, D Mata Sánchez, T Muñoz-Darias, J Sánchez-Sierras, M Armas Padilla, MC Baglio, J Casares, JM Corral-Santana, VA Cúneo, RP Fender, G Ponti, DM Russell, M Shidatsu, D Steeghs, MAP Torres, Y Ueda, F Vincentelli

Professor Rob Fender

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On the distance to the black hole X-ray binary Swift J1727.8$-$1613

Authors:

The Observed Phase Space of Mass-loss History from Massive Stars Based on Radio Observations of a Large Supernova Sample

Authors:

Type I X-ray Bursts Reflected During the X-ray Eclipses of EXO 0748-676

Authors:

The observed phase space of mass-loss history from massive stars based on radio observations of a large supernova sample

Authors:

State-dependent signatures of jets and winds in the optical and infrared spectrum of the black hole transient GX 339$-$4

Authors:

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Professor Rob Fender

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On the distance to the black hole X-ray binary Swift J1727.8$-$1613

Authors:

The Observed Phase Space of Mass-loss History from Massive Stars Based on Radio Observations of a Large Supernova Sample

Authors:

Type I X-ray Bursts Reflected During the X-ray Eclipses of EXO 0748-676

Authors:

The observed phase space of mass-loss history from massive stars based on radio observations of a large supernova sample

Authors:

State-dependent signatures of jets and winds in the optical and infrared spectrum of the black hole transient GX 339$-$4

Authors: