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.

A parsec scale X-ray extended structure from the X-ray binary Circinus X-1

(2008)

Authors:

P Soleri, S Heinz, R Fender, R Wijnands, V Tudose, D Altamirano, PG Jonker, M van der Klis, L Kuiper, C Kaiser, P Casella

High energy astrophysics with the next generation of radio astronomy facilities

(2008)

MAXI, LOFAR and Microquasars - All-sky monitoring of X-ray binaries in X-rays and radio

(2008)

Spectral evidence for jets from Accreting Millisecond X-ray Pulsars

(2008)

Authors:

David M Russell, Rob P Fender, Peter Jonker, Dipankar Maitra

Blazing trails: Microquasars as head-tail sources and the seeding of magnetized plasma into the ISM

(2008)

Authors:

S Heinz, HJ Grimm, RA Sunyaev, RP Fender

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