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.

Jets from X-ray binaries

(2003)

Discovery of type-I X-ray bursts from the low-mass X-ray binary 4U 1708-40

(2003)

Authors:

S Migliari, T Di Salvo, T Belloni, M van der Klis, RP Fender, S Campana, C Kouveliotou, M Méndez, WHG Lewin

Radio/X-ray correlation in the low/hard state of GX 339–4

Astronomy & Astrophysics EDP Sciences 400:3 (2003) 1007-1012

Authors:

S Corbel, MA Nowak, RP Fender, AK Tzioumis, S Markoff

Modeling the X-ray Contribution of X-ray Binary Jets

(2003)

Authors:

S Markoff, M Nowak, S Corbel, R Fender, H Falcke

Radio / X-ray correlation in the low/hard state of GX 339--4

(2003)

Authors:

S Corbel, MA Nowak, RP Fender, AK Tzioumis, S Markoff

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