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.

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

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 318:2 (2000) 599-605

Authors:

Stephan GH Berendsen, Robert Fender, Erik Kuulkers, J Heise, M van der Klis

Giant repeated ejections from GRS 1915+105

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 318:1 (2000) l1-l5

Authors:

RP Fender, GG Pooley

Orbital Dynamics of Cygnus X-3

The Astrophysical Journal American Astronomical Society 541:1 (2000) 308-318

Authors:

MM Hanson, MD Still, RP Fender

Excess submillimetre emission from GRS 1915+105

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 317:1 (2000) 158-162

Authors:

RN Ogley, SJ Bell Burnell, RP Fender, GG Pooley, EB Waltman

The radio luminosity of persistent X-ray binaries

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 317:1 (2000) 1-8

Authors:

RP Fender, MA Hendry

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