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 variable radio counterpart and possible large-scale jet of the new Z source XTE J1701−462

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 380:1 (2007) l25-l29

Authors:

RP Fender, M Dahlem, J Homan, S Corbel, R Sault, TM Belloni

A Highly Polarised Jet in XTE J1748-288

Sissa Medialab Srl (2007) 018

Authors:

Catherine Brocksopp, Rob Fender, James CA Miller-Jones, Ben Stappers

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

Sissa Medialab Srl (2007) 026

Authors:

Sebastian Jester, Elmar Körding, Rob Fender

Deceleration in the radio jets of GRS 1915+105

Sissa Medialab Srl (2007) 060

Authors:

James CA Miller-Jones, Michael Rupen, Rob Fender, Anthony Rushton, Guy G Pooley, Ralph E Spencer

Eight powers of ten: similarities in black hole accretion on all mass scales

Sissa Medialab Srl (2007) 011

Authors:

Rob Fender, Elmar Körding, Tomaso Belloni, Phil Uttley, Ian McHardy, Tasso Tzioumis

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