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.

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

(2008)

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Spectral evidence for jets from Accreting Millisecond X-ray Pulsars

(2008)

Authors:

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

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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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An X-ray Study of the Disc in GX339-4

Sissa Medialab Srl (2008) 015

Authors:

Robert Dunn, Rob Fender, Elmar Körding

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LOFAR Transients and the Radio Sky Monitor

Sissa Medialab Srl (2008) 030

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Professor Rob Fender

Research theme

Sub department

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

Spectral evidence for jets from Accreting Millisecond X-ray Pulsars

Authors:

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

Authors:

An X-ray Study of the Disc in GX339-4

Authors:

LOFAR Transients and the Radio Sky Monitor

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Professor Rob Fender

Research theme

Sub department

Research groups

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

Spectral evidence for jets from Accreting Millisecond X-ray Pulsars

Authors:

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

Authors:

An X-ray Study of the Disc in GX339-4

Authors:

LOFAR Transients and the Radio Sky Monitor