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.

Multiple relativistic outbursts of GRS 1915+105: radio emission and internal shocks

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 363:3 (2005) 867-881

Authors:

JCA Miller-Jones, DG McCormick, RP Fender, RE Spencer, TWB Muxlow, GG Pooley

What can we learn from Neutron Star X-Ray Binaries' JETS?

Astrophysics and Space Science Springer Nature 300:1-3 (2005) 197-209

Authors:

Simone Migliari, Rob Fender

Jets in neutron star X-ray binaries: a comparison with black holes

(2005)

Authors:

S Migliari, RP Fender

Black hole X‐ray binary jets

AIP Conference Proceedings AIP Publishing 797:1 (2005) 189-196

Authors:

Elena Gallo, Rob Fender, Christian Kaiser

Correlation between radio luminosity and X-ray timing frequencies in neutron star and black hole X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 363:1 (2005) 112-120

Authors:

S Migliari, RP Fender, M van der Klis

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