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.

Evidence for deceleration in the radio jets of GRS1915+105?

(2006)

Authors:

JCA Miller-Jones, MP Rupen, RP Fender, A Rushton, GG Pooley, RE Spencer

Active galactic nuclei as scaled-up Galactic black holes

Nature Springer Nature 444:7120 (2006) 730-732

Authors:

IM McHardy, E Koerding, C Knigge, P Uttley, RP Fender

Simultaneous radio/X-ray observations of Cir X-1

(2006)

Authors:

V Tudose, P Soleri, RP Fender, PG Jonker, M van der Klis, AK Tzioumis, RE Spencer

Jet-dominated advective systems of all mass scales

(2006)

Authors:

Elmar Koerding, Rob Fender

A link between radio loudness and X-ray/optical properties of AGN

(2006)

Authors:

Sebastian Jester, Elmar Koerding, Rob Fender

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