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 dark jet dominates the power output of the stellar black hole Cygnus X-1

Nature Springer Nature 436:7052 (2005) 819-821

Authors:

Elena Gallo, Rob Fender, Christian Kaiser, David Russell, Raffaella Morganti, Tom Oosterloo, Sebastian Heinz

Correlation between radio luminosity and X-ray timing frequencies in neutron star and black hole X-ray binaries

(2005)

Authors:

S Migliari, RP Fender, M van der Klis

Energization of interstellar media and cosmic ray production by jets from X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 360:3 (2005) 1085-1090

Authors:

RP Fender, TJ Maccarone, Z Van Kesteren

A unified model for black hole X-ray binary jets ?

(2005)

Authors:

Rob Fender, Tomaso Belloni, Elena Gallo

Discovery of X-ray Jets in the Microquasar H 1743-322

(2005)

Authors:

S Corbel, P Kaaret, RP Fender, AK Tzioumis, JA Tomsick, JA Orosz

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