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.

Infrared spectroscopic variability of Cygnus X-3 in outburst and quiescence

(1999)

Authors:

RP Fender, MM Hanson, GG Pooley

Multiple ejections during the 1975 outburst of A0620-00

(1999)

Authors:

Erik Kuulkers, RP Fender, Ralph E Spencer, Richard J Davis, Ian Morison

Orbital modulation and longer term variability in the radio emission from Cygnus X-1

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 302:1 (1999) l1-l5

Authors:

GG Pooley, RP Fender, C Brocksopp

Infrared spectroscopic variability of Cygnus X-3

Symposium - International Astronomical Union Cambridge University Press (CUP) 193 (1999) 358-359

Authors:

Margaret M Hanson, Rob P Fender, GG Pooley

MERLIN observations of relativistic ejections from GRS 1915+105

(1998)

Authors:

RP Fender, ST Garrington, DJ McKay, TWB Muxlow, GG Pooley, RE Spencer, AM Stirling, EB Waltman

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