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.

Orbital, precessional and flaring variability of Cygnus X-1

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 309:4 (1999) 1063-1073

Authors:

C Brocksopp, RP Fender, V Larionov, VM Lyuty, AE Tarasov, GG Pooley, WS Paciesas, P Roche

Black hole states and radio jet formation

(1999)

A comparison of radio emission from neutron star and black hole X-ray binaries

(1999)

The very flat radio - millimetre spectrum of Cygnus X-1

(1999)

Authors:

RP Fender, GG Pooley, P Durouchoux, RPJ Tilanus, C Brocksopp

Identification of a Likely Radio Counterpart of the Rapid Burster

(1999)

Authors:

CB Moore, RE Rutledge, DW Fox, RA Guerriero, WHG Lewin, R Fender, J van Paradijs

91̽��