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.

Towards a unified model for black hole X-ray binary jets

(2004)

Authors:

RP Fender, TM Belloni, E Gallo

On the Origin of Radio Emission in the X-ray States of XTE J1650-500 during the 2001-2002 Outburst

(2004)

Authors:

S Corbel, RP Fender, JA Tomsick, AK Tzioumis, S Tingay

Correlated X-Ray and Optical Variability in V404 Cygni in Quiescence

The Astrophysical Journal American Astronomical Society 611:2 (2004) l125-l128

Authors:

RI Hynes, PA Charles, MR Garcia, EL Robinson, J Casares, CA Haswell, AKH Kong, M Rupen, RP Fender, RM Wagner, E Gallo, BAC Eves, T Shahbaz, C Zurita

The Correlation between Hard X-Ray Peak Flux and Soft X-Ray Peak Flux in the Outburst Rise of Low-Mass X-Ray Binaries

The Astrophysical Journal American Astronomical Society 611:2 (2004) l121-l124

Authors:

Wenfei Yu, Michiel van der Klis, Rob Fender

Evidence for a Black Hole in the X-ray transient GS 1354-64 (=BW Cir)

(2004)

Authors:

J Casares, C Zurita, T Shahbaz, PA Charles, RP Fender

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