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.

Powerful jets from black hole X-ray binaries in Low/Hard X-ray states

(2000)

The infrared counterpart of the Z source GX 5-1

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 315:4 (2000) l57-l60

Authors:

PG Jonker, RP Fender, NC Hambly, M van der Klis

ASTRONOMY: A New Source of Gamma Rays.

Science American Association for the Advancement of Science (AAAS) 288:5475 (2000) 2326

Giant repeated ejections from GRS 1915+105

(2000)

Authors:

RP Fender, GG Pooley

Simultaneous radio and X-ray observations of Galactic Centre low mass X-ray binaries

(2000)

Authors:

SGH Berendsen, R Fender, E Kuulkers, J Heise, M van der Klis

91̽��