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.

New radio observations of Circinus X-1

(1997)

GRS 1915+105 : Flares, QPOs and other events at 15 GHz

(1997)

Authors:

GG Pooley, RP Fender

High-resolution radio observations of the black hole candidate GX 339-4

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 286:2 (1997) l29-l32

Authors:

RP Fender, RE Spencer, SJ Newell, AK Tzioumis

High-resolution radio observations of GX 339-4

(1997)

Authors:

RP Fender, RE Spencer, SJ Newell, AK Tzioumis

A multiwavelength study of Cygnus X-3

AIP Publishing (1997) 813-817

Authors:

ML McCollough, CR Robinson, SN Zhang, BA Harmon, WS Paciesas, RM Hjellming, M Rupen, AJ Mioduszewski, EB Waltman, RS Foster, FD Ghigo, GG Pooley, RP Fender, W Cui

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