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.

The 1997 hard state outburst of the X-ray transient GS 1354-64 / BW Cir

(2000)

Authors:

C Brocksopp, PG Jonker, RP Fender, PJ Groot, M van der Klis, SJ Tingay

The disc-jet connection in GRS 1915+105

(2000)

Authors:

M Klein-Wolt, RP Fender, GG Pooley, T Belloni, S Migliari, EH Morgan, M van der Klis

Energetics of jets from X-ray binaries

(2000)

A jet model for the broadband spectrum of XTE J1118+480: Synchrotron emission from radio to X-rays in the Low/Hard spectral state

(2000)

Authors:

Sera Markoff, Heino Falcke, Rob Fender

Cygnus X-3 with ISO: investigating the wind

(2000)

Authors:

RN Ogley, SJ Bell Burnell, RP Fender

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