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.

Short-Term Radio-X-ray Correlations of Cygnus X-1

(2003)

Authors:

T Gleissner, J Wilms, GG Pooley, MA Nowak, K Pottschmidt, S Markoff, M Klein-Wolt, RP Fender, R Staubert

A transient large-scale relativistic radio jet from GX 339-4

(2003)

Authors:

Elena Gallo, Stephane Corbel, Rob Fender, Tom Maccarone, Tasso Tzioumis

Chandra Detections of Two Quiescent Black Hole X-Ray Transients

The Astrophysical Journal American Astronomical Society 597:2 (2003) l133-l136

Authors:

John A Tomsick, Stéphane Corbel, Rob Fender, Jon M Miller, Jerome A Orosz, Michael P Rupen, Tasso Tzioumis, Rudy Wijnands, Philip Kaaret

"Soft X-ray transient" outbursts which aren't soft

(2003)

Authors:

C Brocksopp, RM Bandyopadhyay, RP Fender

Evidence of a decrease of kHz quasi-periodic oscillation peak separation towards low frequencies in 4U 1728–34 (GX 354–0)

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 345:3 (2003) l35-l39

Authors:

S Migliari, M van der Klis, RP Fender

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