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.

Chandra imaging spectroscopy of 1E 1740.7 - 2942

(2002)

Authors:

E Gallo, R Fender

Assessing the X-ray Contribution from Jets in X-ray Binaries

(2002)

Authors:

S Markoff, M Nowak, S Corbel, R Fender, H Falcke

The Peculiar Infrared Counterpart of GX 17+2

The Astrophysical Journal American Astronomical Society 574:2 (2002) l143-l146

Authors:

Paul J Callanan, Peter Curran, Alexei V Filippenko, Michael R Garcia, Bruce Margon, Eric Deutsch, Scott Anderson, Lee Homer, Rob P Fender

Do High Frequency QPOs Depend on Phase of Low Frequency QPOs in XTE J1550-564 ?

(2002)

Authors:

W Yu, M van der Klis, R Fender

On the correlation between radio and X-ray flux in Low/Hard state Black Holes

(2002)

Authors:

E Gallo, R Fender, G Pooley

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