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.

Disk mass accretion rate and infrared flares in GRS 1915+105

(2000)

Authors:

T Belloni, S Migliari, RP Fender

The infrared counterpart of the Z source GX5-1

(2000)

Authors:

Peter G Jonker, Rob P Fender, Nigel C Hambly, Michiel van der Klis

Orbital dynamics of Cygnus X-3

(2000)

Authors:

MM Hanson, MD Still, RP Fender

Resolving the radio nebula around beta Lyrae

(2000)

Authors:

G Umana, PFL Maxted, C Trigilio, RP Fender, F Leone, SK Yerli

Excess sub-millimetre emission from GRS 1915+105

(2000)

Authors:

RN Ogley, SJ Bell Burnell, RP Fender, GG Pooley, EB Waltman

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