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.

A Global Spectral 51�� of Black Hole X-ray Binaries

(2009)

Authors:

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

A long-term optical - X-ray correlation in 4U 1957+11

(2009)

Authors:

DM Russell, F Lewis, P Roche, JS Clark, E Breedt, RP Fender

Correlated radio/X-ray behaviour of Cyg X-3

Sissa Medialab Srl (2009) 018

Authors:

V Tudose, James CA Miller-Jones, Rob Fender, Zsolt Paragi, Charli Sakari, Anna Szostek, Michael Garrett, Vivek Dhawan, Anthony Rushton, Ralph E Spencer, M van der Klis

The LOFAR Transients Key Science Project (invited)

Sissa Medialab Srl (2009) 021

Authors:

Ben Stappers, Rob Fender, Ralph AMJ Wijers

The proper motion and changing jet morphology of Cygnus X-3

Sissa Medialab Srl (2009) 017

Authors:

James CA Miller-Jones, Charli Sakari, Vivek Dhawan, Valeriu M Tudose, Rob Fender, Zsolt Paragi, Michael Garrett

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