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.

Unifying disc-jet behaviour in X-ray binaries: an optical/IR approach

(2008)

Authors:

David M Russell, Dipankar Maitra, Rob P Fender, Fraser Lewis

Continued Monitoring of LMXBs with the Faulkes Telescopes

(2008)

Authors:

Fraser Lewis, David M Russell, Rob P Fender, Paul Roche, J Simon Clark

A Global 51�� of X-ray Binaries

(2008)

Authors:

Robert Dunn, Rob Fender, Elmar Koerding, Clement Cabanac, Tomaso Belloni

Spectral evidence for jets from Accreting Millisecond X‐ray Pulsars

AIP Conference Proceedings AIP Publishing 1068:1 (2008) 221-224

Authors:

DM Russell, RP Fender, P Jonker, D Maitra, Rudy Wijnands, Diego Altamirano, Paolo Soleri, Nathalie Degenaar, Nanda Rea, Piergiorgio Casella, Alessandro Patruno, Manuel Linares

Broad-band X-ray spectral evolution of GX 339-4 during a state transition

(2008)

Authors:

M Del Santo, TM Belloni, J Homan, A Bazzano, P Casella, RP Fender, E Gallo, N Gehrels, WHG Lewin, M Mendez, M van der Klis

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